The Science of the Einstein Telescope

Abstract

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science objectives, providing state-of-the-art predictions for the capabilities of ET in both geometries currently under consideration, a single-site triangular configuration or two L-shaped detectors. We discuss the impact that ET will have on domains as broad and diverse as fundamental physics, cosmology, early Universe, astrophysics of compact objects, physics of matter in extreme conditions, and dynamics of stellar collapse. We discuss how the study of extreme astrophysical events will be enhanced by multi-messenger observations. We highlight the ET synergies with ground-based and space-borne GW observatories, including multi-band investigations of the same sources, improved parameter estimation, and complementary information on astrophysical or cosmological mechanisms obtained combining observations from different frequency bands. We present advancements in waveform modeling dedicated to third-generation observatories, along with open tools developed within the ET Collaboration for assessing the scientific potentials of different detector configurations. We finally discuss the data analysis challenges posed by third-generation observatories, which will enable access to large populations of sources and provide unprecedented precision.

899 pages, 205 figures, v2: minor improvements, the version to appear in JCAP

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• Gravitational Waves from Phase Transitions at the Electroweak Scale and Beyond
• Kilonovae
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• Population III star formation in a Lambda CDM universe, I: The effect of formation redshift and environment on protostellar accretion rate
• Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope
• Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
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• Towards models of gravitational waveforms from generic binaries: A simple approximate mapping between precessing and non-precessing inspiral signals
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• Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits
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• Dynamical evolution of black hole sub-systems in idealised star clusters
• Magnetized Neutron Star Mergers and Gravitational Wave Signals
• Maximum elastic deformations of relativistic stars
• A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
• Predicting the direction of the final spin from the coalescence of two black holes
• Reducing orbital eccentricity in binary black hole simulations
• Classical and quantum scattering in post-Minkowskian gravity
• An Open-Source Neutrino Radiation Hydrodynamics Code for Core-Collapse Supernovae
• Primordial black holes with an accurate QCD equation of state
• Lower bound on the primordial black hole merger rate
• FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis
• Testing local Lorentz invariance with gravitational waves
• LISA detections of massive black hole inspirals: parameter extraction errors due to inaccurate template waveforms
• The Low-Energy Effective Theory of Axions and ALPs
• Bayesian parameter estimation using conditional variational autoencoders for gravitational-wave astronomy
• MICROSCOPE mission: first constraints on the violation of the weak equivalence principle by a light scalar dilaton
• Cosmology with the lights off: Standard sirens in the Einstein Telescope era
• An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451
• Disordered nuclear pasta, magnetic field decay, and crust cooling in neutron stars
• The gravitational-wave luminosity distance in modified gravity theories
• Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
• The THESEUS space mission concept: science case, design and expected performances
• Next to Leading Order Spin(1)Spin(1) Effects in the Motion of Inspiralling Compact Binaries
• Massively parallel Bayesian inference for transient gravitational-wave astronomy
• The anisotropic power spectrum and bispectrum in the f(phi) F^2 mechanism
• Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100)
• A ~50,000 solar mass black hole in the nucleus of RGG 118
• The Juelich hyperon-nucleon model revisited
• Constraining Dark Matter candidates from structure formation
• Demographics of the Galaxies Hosting Short-duration Gamma-Ray Bursts
• Spectral Representations of Neutron-Star Equations of State
• Harmonic coordinate method for simulating generic singularities
• Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA
• Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models
• Low mass binary neutron star mergers : gravitational waves and neutrino emission
• Compact Binary Coalescences in the Band of Ground-based Gravitational-Wave Detectors
• Accurate evolutions of inspiralling and magnetized neutron-stars: equal-mass binaries
• Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
• Charged-current weak interaction processes in hot and dense matter and its impact on the spectra of neutrinos emitted from proto-neutron star cooling
• A Decline in the X-ray through Radio Emission from GW170817 Continues to Support an Off-Axis Structured Jet
• Scattering Amplitudes, the Tail Effect, and Conservative Binary Dynamics at $O(G^4)$
• Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
• Non-parametric inference of the neutron star equation of state from gravitational wave observations
• Double neutron stars: merger rates revisited
• Constraints on Einstein-Æther theory and Horava gravity from binary pulsar observations
• The observed velocity distribution of young pulsars
• TIGER: A data analysis pipeline for testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing compact binaries
• Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
• Mode sum regularization approach for the self-force in black hole spacetime
• The Pacific Ocean Neutrino Experiment
• Strong CP problem and mirror world: the Weinberg Wilczek axion revisited
• Post-Newtonian, Quasi-Circular Binary Inspirals in Quadratic Modified Gravity
• An intermediate-mass black hole in the centre of the globular cluster 47 Tucanae
• A Sun-like star orbiting a black hole
• Compact binary evolutions with the Z4c formulation
• Hierarchical analysis of gravitational-wave measurements of binary black hole spin-orbit misalignments
• Georgia Tech Catalog of Gravitational Waveforms
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
• GLADE: A Galaxy Catalogue for Multi-Messenger Searches in the Advanced Gravitational-Wave Detector Era
• Inverse cascade in decaying 3D magnetohydrodynamic turbulence
• Observation of Gravitational Waves from the Coalescence of a $2.5\text{-}4.5M_{\odot }$ Compact Object and a Neutron Star
• A Periodic Table for Black Hole Orbits
• Analytical solutions of bound timelike geodesic orbits in Kerr spacetime
• Observational Evidence for Primordial Black Holes: A Positivist Perspective
• Spin(1)Spin(2) Effects in the Motion of Inspiralling Compact Binaries at Third Order in the Post-Newtonian Expansion
• On the birthrates of Galactic neutron stars
• Probing non-tensorial polarizations of stochastic gravitational-wave backgrounds with ground-based laser interferometers
• GW190814: Impact of a 2.6 solar mass neutron star on nucleonic equations of state
• The Spectral SN-GRB Connection: Systematic Spectral Comparisons between Type Ic Supernovae, and broad-lined Type Ic Supernovae with and without Gamma-Ray Bursts
• Medium modification of the charged current neutrino opacity and its implications
• Dissipative Effects in the Worldline Approach to Black Hole Dynamics
• Universal infrared scaling of gravitational wave background spectra
• Sound shell model for acoustic gravitational wave production at a first-order phase transition in the early Universe
• Constraints on cosmic strings using data from the third Advanced LIGO-Virgo observing run
• Neutrino-driven convection versus advection in core collapse supernovae
• Masses and Scaling Relations for Nuclear Star Clusters, and their Coexistence with Central Black Holes
• The Pair-Instability Mass Gap for Black Holes
• Dynamics of Binary Systems to Fourth Post-Minkowskian Order from the Effective Field Theory Approach
• Observational Black Hole Spectroscopy: A time-domain multimode analysis of GW150914
• Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
• Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform
• Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of ${}^{208}$Pb with Minimal Modeling Assumptions
• Where are LIGO's Big Black Holes?
• Hydrodynamics of core-collapse supernovae and their progenitors
• Signatures of hypermassive neutron star lifetimes on r-process nucleosynthesis in the disk ejecta from neutron star mergers
• A Comparison of Intermediate Mass Black Hole Candidate ULXs and Stellar-Mass Black Holes
• Gauge field production in SUGRA inflation: local non-Gaussianity and primordial black holes
• Core-Collapse Supernovae and Host Galaxy Stellar Populations
• Theory-Agnostic Constraints on Black-Hole Dipole Radiation with Multi-Band Gravitational-Wave Astrophysics
• Modified gravitational-wave propagation and standard sirens
• Gravitational-wave cosmology across 29 decades in frequency
• Binary-black-hole initial data with nearly-extremal spins
• Early seeds of axion miniclusters
• The Timing of Nine Globular Cluster Pulsars
• Bayesian model selection for testing the no-hair theorem with black hole ringdowns
• Black hole and neutron star mergers in galactic nuclei
• Linearized f(R) Gravity: Gravitational Radiation & Solar System Tests
• Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation
• On the estimation of gravitational wave spectrum from cosmic domain walls
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes
• Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
• Constructing Gravitational Waves from Generic Spin-Precessing Compact Binary Inspirals
• Gravitational Recoil From Accretion-Aligned Black-Hole Binaries
• Properties of hypermassive neutron stars formed in mergers of spinning binaries
• The imprint of massive black hole formation models on the LISA data stream
• Gravitational Waves from Warped Spacetime
• POSSIS: predicting spectra, light curves and polarization for multi-dimensional models of supernovae and kilonovae
• The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole
• New Developments in Flavor Evolution of a Dense Neutrino Gas
• Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio
• Recent Progress in the Physics of Axions and Axion-Like Particles
• Including higher order multipoles in gravitational-wave models for precessing binary black holes
• The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_{\odot }$ Stars
• High-resolution magnetohydrodynamics simulation of black hole-neutron star merger: Mass ejection and short gamma-ray burst
• Postmerger Gravitational-Wave Signatures of Phase Transitions in Binary Mergers
• Notes on the integration of numerical relativity waveforms
• The Explosion of Helium Stars Evolved With Mass Loss
• The Evolution of Galaxy Number Density at z < 8 and its Implications
• General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star
• Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source
• Self-consistent 3D Supernova Models From -7 Minutes to +7 Seconds: a 1-bethe Explosion of a ~19 Solar-mass Progenitor
• Fourth post-Newtonian effective one-body dynamics
• Equation-of-state-independent relations in neutron stars
• Gravitational radiation from an axion cloud around a black hole: Superradiant phase
• Choked Jets and Low-Luminosity Gamma-Ray Bursts as Hidden Neutrino Sources
• Black hole mergers from an evolving population of globular clusters
• A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries
• Phasing of gravitational waves from inspiralling eccentric binaries
• Spontaneous Scalarization with Massive Fields
• Simulations of Binary Black Hole Mergers Using Spectral Methods
• Nebular emission-line profiles of Type Ib/c Supernovae - probing the ejecta asphericity
• A Rigorous Derivation of Gravitational Self-force
• A Successful 3D Core-Collapse Supernova Explosion Model
• The Normal Law Under Linear Restrictions: Simulation and Estimation via Minimax Tilting
• Black holes and binary mergers in scalar Gauss-Bonnet gravity: scalar field dynamics
• Compact stars with sequential QCD phase transitions
• A review of gravitational waves from cosmic domain walls
• Full Transport Model of GW170817-Like Disk Produces a Blue Kilonova
• Gravitational self-force on a particle in eccentric orbit around a Schwarzschild black hole
• Primordial Black Holes Confront LIGO/Virgo data: Current situation
• Coalescence of binary neutron stars in a scalar-tensor theory of gravity
• Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae
• Radiative contribution to classical gravitational scattering at the third order in $G$
• Massive Stars in the Range $13-25{\mathrm{M}}_{\odot }$: Evolution and Nucleosynthesis. II. the Solar Metallicity Models
• The gravitational wave signal from core-collapse supernovae
• Calculating the gravitational self force in Schwarzschild spacetime
• The ephemeris, orbital decay, and masses of 10 eclipsing HMXBs
• Production of the entire range of r-process nuclides by black hole accretion disc outflows from neutron star mergers
• Efficiency of mass transfer in massive close binaries, Tests from double-lined eclipsing binaries in the SMC
• From Boundary Data to Bound States II: Scattering Angle to Dynamical Invariants (with Twist)
• How much 56Ni can be produced in Core-Collapse Supernovae? : Evolution and Explosions of 30 - 100 Msun Stars
• LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources
• Exploring properties of high-density matter through remnants of neutron-star mergers
• Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae
• Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions
• Gravitational waves from inspiraling compact binaries: Validity of the stationary-phase approximation to the Fourier transform
• Distinguishing Boson Stars from Black Holes and Neutron Stars from Tidal Interactions in Inspiraling Binary Systems
• Dynamical scalarization of neutron stars in scalar-tensor gravity theories
• A highly resistive layer within the crust of X-ray pulsars limits their spin periods
• Time-Reversal Breaking in QCD${}_4$, Walls, and Dualities in 2+1 Dimensions
• Black Hole Mergers From Globular Clusters Observable by LISA I: Eccentric Sources Originating From Relativistic $N$-body Dynamics
• The Kerr Metric
• Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
• Quantum Monte Carlo calculation of the equation of state of neutron matter
• Stability of mass transfer from massive giants: double black-hole binary formation and ultra-luminous X-ray sources
• A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism
• Fast and Accurate Inference on Gravitational Waves from Precessing Compact Binaries
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
• Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions
• Extending the search for muon neutrinos coincident with gamma-ray bursts in IceCube data
• How perturbative QCD constrains the Equation of State at Neutron-Star densities
• Seeding primordial black holes in multifield inflation
• Degeneracy between mass and spin in black-hole-binary waveforms
• Nearby Supernova Rates from the Lick Observatory Supernova Search. I. The Methods and Database
• Vorticity, kinetic energy, and suppressed gravitational wave production in strong first order phase transitions
• The Search for Failed Supernovae with The Large Binocular Telescope: First Candidates
• Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description
• Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order
• Constraining twin stars with GW170817
• Mergers of Stellar-Mass Black Holes in Nuclear Star Clusters
• On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening
• Black holes in an Effective Field Theory extension of GR
• Symmetry energy impact in simulations of core-collapse supernovae
• The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data
• Scale-dependent gravitational waves from a rolling axion
• Relativistic simulations of black hole-neutron star coalescence: the jet emerges
• Progenitor mass constraints for core-collapse supernovae from correlations with host galaxy star formation
• The role of mass transfer and common envelope evolution in the formation of merging binary black holes
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
• Detection of Neutrinos from Supernovae in Nearby Galaxies
• High-Order Fully General-Relativistic Hydrodynamics: new Approaches and Tests
• On the nuclear robustness of the r process in neutron-star mergers
• Multi-messenger picture of compact binary mergers
• Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations
• Black holes and the multiverse
• A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries
• The Ineludible non-Gaussianity of the Primordial Black Hole Abundance
• Tracking the precession of compact binaries from their gravitational-wave signal
• Chiral Effective Field Theory and the High-Density Nuclear Equation of State
• Two populations of metal-free stars in the early Universe
• Gravitational waves from first order cosmological phase transitions in the Sound Shell Model
• Growth of structure seeded by primordial black holes
• The Initial Spin Probability Distribution of Primordial Black Holes
• Floating and sinking: the imprint of massive scalars around rotating black holes
• Constraints on cosmic strings using data from the first Advanced LIGO observing run
• Gravitational Waves from Neutron Stars: A Review
• Nonlinearities in Black Hole Ringdowns
• Gravitational waves from spinning black hole-neutron star binaries: dependence on black hole spins and on neutron star equations of state
• Stochastic Gravitational Wave Background from Coalescing Binary Black Holes
• Addressing the spin question in gravitational-wave searches: Waveform templates for inspiralling compact binaries with nonprecessing spins
• A year in the life of GW170817: the rise and fall of a structured jet from a binary neutron star merger
• R-process Nucleosynthesis from Three-Dimensional Magnetorotational Core-Collapse Supernovae
• The Hyperfine Einstein-Infeld-Hoffmann Potential
• Conservative Dynamics of Binary Systems at Fourth Post-Minkowskian Order in the Large-eccentricity Expansion
• Magnetorotational instability in relativistic hypermassive neutron stars
• Interacting Supernovae: Types IIn and Ibn
• Can very compact and very massive neutron stars both exist?
• The environment of the binary neutron star merger GW170817
• Nonlinear effects in black hole ringdown
• Beyond second-order convergence in simulations of binary neutron stars in full general-relativity
• Enhancing Gravitational-Wave Science with Machine Learning
• Constraining the Statistics of Population III Binaries
• Neutrino-driven wind simulations and nucleosynthesis of heavy elements
• Models of Kilonova/macronova emission from black hole-neutron star mergers
• A Comprehensive Study of Neutron Star Retention in Globular Clusters
• ZAIGA: Zhaoshan Long-baseline Atom Interferometer Gravitation Antenna
• Searching for a subpopulation of primordial black holes in LIGO/Virgo gravitational-wave data
• Observing Gravitational Waves From The Post-Merger Phase Of Binary Neutron Star Coalescence
• Low significance of evidence for black hole echoes in gravitational wave data
• Compact binary systems in scalar-tensor gravity: Equations of motion to 2.5 post-Newtonian order
• Early evolution of newly born magnetars with a strong toroidal field
• Cosmological Consequences of Nearly Conformal Dynamics at the TeV scale
• Systematic study of magnetar outbursts
• Early Structure Formation in $\Lambda$PBH Cosmologies
• The host galaxies of core-collapse supernovae and gamma ray bursts
• Tidal Deformation and Dissipation of Rotating Black Holes
• Accurate precision Cosmology with redshift unknown gravitational wave sources
• Primordial Gravitational Waves from Axion-Gauge Fields Dynamics
• Radiation Reaction and Gravitational Waves at Fourth Post-Minkowskian Order
• Asymmetric Supernovae from Magneto-Centrifugal Jets
• Non-Gaussianities and chiral gravitational waves in natural steep inflation
• Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background
• Initial mass function of intermediate mass black hole seeds
• The Formation Rates of Population III Stars and Chemical Enrichment of Halos during the Reionization Era
• Super-AGB Stars and their role as Electron Capture Supernova progenitors
• Unequal mass binary neutron star mergers and multimessenger signals
• Energetics of two-body Hamiltonians in post-Minkowskian gravity
• Gravitational-wave parameter estimation with autoregressive neural network flows
• Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
• A Short GRB "No-Host'' Problem? Investigating Large Progenitor Offsets for Short GRBs with Optical Afterglows
• Primordial black hole formation and abundance: contribution from the non-linear relation between the density and curvature perturbation
• Revealing the high-density equation of state through binary neutron star mergers
• The impact of pair-instability mass loss on the binary black hole mass distribution
• Improved Dynamical Constraints on the Masses of the Central Black Holes in Nearby Low-mass Early-type Galactic Nuclei And the First Black Hole Determination for NGC 205
• Bosonic Dark Matter in Neutron Stars and its Effect on Gravitational Wave Signal
• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• Primordial black hole production during first-order phase transitions
• Reference Database for Photon Strength Functions
• I-Love-Q, Spontaneously: Slowly Rotating Neutron Stars in Scalar-Tensor Theories
• The formation and hierarchical assembly of globular cluster populations
• Testing post-Newtonian theory with gravitational wave observations
• An improved analysis of GW150914 using a fully spin-precessing waveform model
• Black Holes' Dark Dress: On the merger rate of a subdominant population of primordial black holes
• Constraints on binary neutron star merger product from short GRB observations
• Dark matter substructure and dwarf galactic satellites
• Next-to-next-to-leading order spin-orbit effects in the gravitational wave flux and orbital phasing of compact binaries
• Constraining Formation Models of Binary Black Holes with Gravitational-Wave Observations
• Head-on collisions of boson stars
• Thermodynamics conditions of matter in neutron star mergers
• On the nature of massive helium star winds and Wolf-Rayet-type mass loss
• Extreme- and Intermediate-Mass Ratio Inspirals in Dynamical Chern-Simons Modified Gravity
• The BayesWave analysis pipeline in the era of gravitational wave observations
• Probing the pre-BBN universe with gravitational waves from cosmic strings
• A new probe of dark matter properties: gravitational waves from an intermediate mass black hole embedded in a dark matter mini-spike
• Absorption of mass and angular momentum by a black hole: Time-domain formalisms for gravitational perturbations, and the small-hole/slow-motion approximation
• Probing the non-linear structure of general relativity with black hole binaries
• Beyond the Standard Models with Cosmic Strings
• Combined Constraints on the Equation of State of Dense Neutron-Rich Matter from Terrestrial Experiments and Observations of Neutron Stars
• Unified treatment of sub-saturation stellar matter at zero and finite temperature
• Relic Backgrounds of Gravitational Waves from Cosmic Turbulence
• Detectability of compact binary merger macronovae
• Axion cosmology with long-lived domain walls
• Distinguishing Between Formation Channels for Binary Black Holes with LISA
• High-resolution supernova neutrino spectra represented by a simple fit
• Search for Supernova Neutrino Bursts at Super-Kamiokande
• Unified equation of state for neutron stars on a microscopic basis
• Periastron Advance in Black-Hole Binaries
• New Class of High-Energy Transients from Crashes of Supernova Ejecta with Massive Circumstellar Material Shells
• Ram-pressure stripping of a kicked Hill sphere: Prompt electromagnetic emission from the merger of stellar mass black holes in an AGN accretion disk
• Gravitational and electromagnetic outputs from binary neutron star mergers
• Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase
• A Mock Data Challenge for the Einstein Gravitational-Wave Telescope
• Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts
• Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
• Testing the binary black hole nature of a compact binary coalescence
• Gravitational Waves from the Remnants of the First Stars
• A Challenge to the Standard Cosmological Model
• Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up and ${}^{12}$C($\alpha$, $\gamma$)${}^{16}$O rate on the pair-instability black hole mass gap
• The optical afterglow of GW170817 at one year post-merger
• General relativistic simulations of compact binary mergers as engines of short gamma-ray bursts
• Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties
• Radio Detections During Two State Transitions of the Intermediate Mass Black Hole HLX-1
• Nested sampling for physical scientists
• Ready-to-use post-Newtonian gravitational waveforms for binary black holes with non-precessing spins: An update
• Testing Seesaw and Leptogenesis with Gravitational Waves
• Gravitational Waves from Core Collapse Supernovae
• A Surrogate Model of Gravitational Waveforms from Numerical Relativity Simulations of Precessing Binary Black Hole Mergers
• It has to be cool: on supergiant progenitors of binary black hole mergers from common-envelope evolution
• Stability analysis of chromo-natural inflation and possible evasion of Lyth's bound
• Geometry and Regularity of Moving Punctures
• Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers
• Precision cosmology from future lensed gravitational wave and electromagnetic signals
• Revealing the Supernova--Gamma-Ray Burst Connection with TeV Neutrinos
• Non-perturbative and self-consistent models of neutron stars in R-squared gravity
• Anomalous solutions to the strong CP problem
• Primordial black hole evolution in tensor-scalar cosmology
• The impact of mass-transfer physics on the observable properties of field binary black hole populations
• Mountains on Neutron Stars: Accreted vs. Non-Accreted crusts
• Strong Binary Pulsar Constraints on Lorentz Violation in Gravity
• Gravitational Waves from Quasicircular Extreme Mass-Ratio Inspirals as Probes of Scalar-Tensor Theories
• Anisotropic stars as ultracompact objects in General Relativity
• Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations
• Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog
• The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries
• Observing Gravitational Waves from Core-Collapse Supernovae in the Advanced Detector Era
• Global Comparison of Core-Collapse Supernova Simulations in Spherical Symmetry
• On the rate of core collapse supernovae in the Milky Way
• A red giant orbiting a black hole
• The Asiago Supernova Catalogue- 10 years after
• Gravitational waves from vacuum first order phase transitions II: from thin to thick walls
• Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy
• The expansion of stripped-envelope stars: consequences for supernovae and gravitational-wave progenitors
• Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters
• Agnostic black hole spectroscopy: Quasinormal mode content of numerical relativity waveforms and limits of validity of linear perturbation theory
• Nuclear Equation of State from Observations of Short Gamma-Ray Burst Remnants
• Gravitational Radiation from Newborn Magnetars
• Extracting equation of state parameters from black hole-neutron star mergers. I. Nonspinning black holes
• The redshift evolution of the binary black hole merger rate: a weighty matter
• Next-to-next-to-leading order spin-orbit effects in the near-zone metric and precession equations of compact binaries
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• On the importance of heavy fields during inflation
• A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
• Dynamical r-process studies within the neutrino-driven wind scenario and its sensitivity to the nuclear physics input
• General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers
• On the Rate of Neutron Star Binary Mergers from Globular Clusters
• Estimates for Disk and Ejecta Masses Produced in Compact Binary Mergers
• Gravitational waves as a probe of dark matter mini-spikes
• Black Hole and Neutron Star Binary Mergers in Triple Systems: Merger Fraction and Spin-Orbit Misalignment
• Gravitational waveforms for compact binaries from second-order self-force theory
• Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach II: Renormalized Lagrangian
• Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
• The Progenitor of Supernova 2011dh/PTF11eon in Messier 51
• Precise LIGO Lensing Rate Predictions for Binary Black Holes
• Signatures of a jet cocoon in early spectra of a supernova associated with a $\gamma$-ray burst
• Fokker action of non-spinning compact binaries at the fourth post-Newtonian approximation
• The MBTA Pipeline for Detecting Compact Binary Coalescences in the Third LIGO-Virgo Observing Run
• A stochastic template placement algorithm for gravitational wave data analysis
• Second-order self-force calculation of the gravitational binding energy in compact binaries
• Second-order gravitational self-force
• Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
• Gravitational wave bursts from cosmic (super)strings: Quantitative analysis and constraints
• Low-metallicity massive single stars with rotation. Evolutionary models applicable to I Zwicky 18
• A multipolar effective one body waveform model for spin-aligned black hole binaries
• Improved reconstruction of a stochastic gravitational wave background with LISA
• On the number density of "direct collapse" black hole seeds
• Convolutional neural networks: a magic bullet for gravitational-wave detection?
• Reducing phase error in long numerical binary black hole evolutions with sixth order finite differencing
• Numerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and Nucleosynthesis
• Neutron-star Radius from a Population of Binary Neutron Star Mergers
• Conservative dynamics of two-body systems at the fourth post-Newtonian approximation of general relativity
• The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
• Primordial black hole and wormhole formation by domain walls
• Holographic Operator Mixing and Quasinormal Modes on the Brane
• Gravitational radiation reaction and inspiral waveforms in the adiabatic limit
• Numerical Simulations of Gravitational Waves from Early-Universe Turbulence
• New constraints on primordial gravitational waves from Planck 2015
• A General-relativistic Determination of the Threshold Mass to Prompt Collapse in Binary Neutron Star Mergers
• Gravitational Radiation from an Accreting Millisecond Pulsar with a Magnetically Confined Mountain
• Stochastic backgrounds in alternative theories of gravity: overlap reduction functions for pulsar timing arrays
• The relativistic pulsar-white dwarf binary PSR J1738+0333 I. Mass determination and evolutionary history
• Pre-supernova evolution, compact object masses and explosion properties of stripped binary stars
• Multimessenger Signatures of Massive Black Holes in Dwarf Galaxies
• Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes
• A NICER view of PSR J0030+0451: evidence for a global-scale multipolar magnetic field
• Resonant Tidal Excitations of Rotating Neutron Stars in Coalescing Binaries
• Populating the upper black hole mass gap through stellar collisions in young star clusters
• QCD-Electroweak First-Order Phase Transition in a Supercooled Universe
• Gravitational self force on a particle in circular orbit around a Schwarzschild black hole
• Probing Planckian corrections at the horizon scale with LISA binaries
• GW190521 as a dynamical capture of two nonspinning black holes
• The GW190521 Mass Gap Event and the Primordial Black Hole Scenario
• Breaking stress of neutron star crust
• An effective formalism for testing extensions to General Relativity with gravitational waves
• Effective one body multipolar waveform model for spin-aligned, quasi-circular, eccentric, hyperbolic black hole binaries
• Tidal deformability with sharp phase transitions in (binary) neutron stars
• Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals
• The Origin of Black Hole Spin in Galactic Low-Mass X-ray Binaries
• Short-lived ${}^{244}$Pu Points to Compact Binary Mergers as Sites for Heavy r-process Nucleosynthesis
• Evolution of inspiral orbits around a Schwarzschild black hole
• Extracting equation of state parameters from black hole-neutron star mergers: aligned-spin black holes and a preliminary waveform model
• Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
• Black-hole Spectroscopy by Making Full Use of Gravitational-Wave Modeling
• Quasinormal modes of Einstein-Gauss-Bonnet-dilaton black holes
• Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation
• The Role of Magnetic Field Geometry in the Evolution of Neutron Star Merger Accretion Discs
• Factoring the Strong CP Problem
• Identification and mitigation of narrow spectral artifacts that degrade searches for persistent gravitational waves in the first two observing runs of Advanced LIGO
• The tail effect in gravitational radiation-reaction: time non-locality and renormalization group evolution
• Spinning Black Holes Fall in Love
• Gravitational radiation reaction along general orbits in the effective one-body formalism
• Binary black holes in young star clusters: the impact of metallicity
• The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
• Analytic Description of Primordial Black Hole Formation from Scalar Field Fragmentation
• Sixth post-Newtonian local-in-time dynamics of binary systems
• Hunting for Dark Particles with Gravitational Waves
• Astronuclear Physics: a Tale of the Atomic Nuclei in the Skies
• Constraining the high redshift formation of black hole seeds in nuclear star clusters with gas inflows
• Self-interaction spin effects in inspiralling compact binaries
• Mass-gap Mergers in Active Galactic Nuclei
• Revising the multipole moments of numerical spacetimes, and its consequences
• Cosmic Archaeology with Gravitational Waves from Cosmic Strings
• Towards an all-orders calculation of the electroweak bubble wall velocity
• On the mass radiated by coalescing black-hole binaries
• High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants
• A Model of Visible QCD Axion
• The Evolution of Primordial Black Holes and their Final Observable Spins
• Nested Sampling with Normalising Flows for Gravitational-Wave Inference
• Globular Cluster Formation and Evolution in the Context of Cosmological Galaxy Assembly: Open Questions
• Neutrino and axion emissivities of neutron stars from nucleon-nucleon scattering data
• Binary black holes in the pair-instability mass gap
• Primordial black hole formation in the matter-dominated phase of the Universe
• Neutrino oscillations in supernovae: angular moments and fast instabilities
• Cosmic string loop distribution on all length scales and at any redshift
• Exploring the Bayesian parameter estimation of binary black holes with LISA
• Dynamics of spontaneous black hole scalarization and mergers in Einstein-scalar-Gauss-Bonnet gravity
• Prototype Global Analysis of LISA Data with Multiple Source Types
• The evolution of stellar triples: The most common evolutionary pathways
• Probing Extreme-Density Matter with Gravitational Wave Observations of Binary Neutron Star Merger Remnants
• Gravitational-wave phasing for low-eccentricity inspiralling compact binaries to 3PN order
• Tidal Love Numbers of Kerr Black Holes
• Third post-Newtonian angular momentum flux and the secular evolution of orbital elements for inspiralling compact binaries in quasi-elliptical orbits
• New derivation of a third post-Newtonian equation of motion for relativistic compact binaries without ambiguity
• Equation of State Effects on Gravitational Waves from Rotating Core Collapse
• A New Gravitational-Wave Signature from Standing Accretion Shock Instabilities in Supernovae
• Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency
• Astrophysical and theoretical physics implications from multimessenger neutron star observations
• The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range
• Perturbative Thermal QCD: Formalism and Applications
• X-Pipeline: An analysis package for autonomous gravitational-wave burst searches
• Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach I: Regularized Lagrangian
• Primordial non-gaussianity up to all orders: theoretical aspects and implications for primordial black hole models
• Conservative Tidal Effects in Compact Binary Systems to Next-to-Leading Post-Minkowskian Order
• Effects of waveform model systematics on the interpretation of GW150914
• First 100 ms of a long-lived magnetized neutron star formed in a binary neutron star merger
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• Searching for Dark Photon Dark Matter with Gravitational Wave Detectors
• WIMPs and stellar-mass primordial black holes are incompatible
• LOSS Revisited - II: The relative rates of different types of supernovae vary between low- and high-mass galaxies
• Consistent neutron star models with magnetic field dependent equations of state
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• Exploring the Lower Mass Gap and Unequal Mass Regime in Compact Binary Evolution
• Multi-timescale analysis of phase transitions in precessing black-hole binaries
• Eccentric Black Hole Mergers in Active Galactic Nuclei
• Circular orbits and spin in black-hole initial data
• Gravitational Collider Physics
• Star clusters near and far; tracing star formation across cosmic time
• Speed of Gravitational Waves from Strongly Lensed Gravitational Waves and Electromagnetic Signals
• From the first stars to the first black holes
• Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817
• Dynamics and Gravitational Wave Signature of Collapsar Formation
• Explosion geometry of a rotating 13 $M_{\odot }$ star driven by the SASI-aided neutrino-heating supernova mechanism
• Solving puzzles of GW150914 by primordial black holes
• Numerical binary black hole mergers in dynamical Chern-Simons: I. Scalar field
• Phantom dark energy from non-local infrared modifications of General Relativity
• Equation of state and thickness of the inner crust of neutron stars
• CMB constraints on cosmic strings and superstrings
• Direct constraints on ultra-light boson mass from searches for continuous gravitational waves
• The Tune of Love and the Nature(ness) of Spacetime
• Oscillations in the stochastic gravitational wave background from sharp features and particle production during inflation
• The Crab Nebula and the class of Type IIn-P supernovae caused by sub-energetic electron capture explosions
• Phase effects from strong gravitational lensing of gravitational waves
• Super-Eddington growth of the first black holes
• JWST/NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
• Parametrized 3D models of neutrino-driven supernova explosions: Neutrino emission asymmetries and gravitational-wave signals
• Core-collapse supernovae missed by optical surveys
• Inspiralling compact binaries in quasi-elliptical orbits: The complete third post-Newtonian energy flux
• Spin Effects in the Effective Field Theory Approach to Post-Minkowskian Conservative Dynamics
• Towards adiabatic waveforms for inspiral into Kerr black holes: I. A new model of the source for the time domain perturbation equation
• Producing Magnetar Magnetic Fields in the Merger of Binary Neutron Stars
• From inflation to black hole mergers and back again: Gravitational-wave data-driven constraints on inflationary scenarios with a first-principle model of primordial black holes across the QCD epoch
• Primordial black hole formation with non-Gaussian curvature perturbations
• Merger of black hole and neutron star in general relativity: Tidal disruption, torus mass, and gravitational waves
• The Birth of a Massive First-Star Binary
• (No) neutron star maximum mass constraint from hypernuclei
• Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies
• Formation Rates and Evolution Histories of Magnetars
• Direct Astrophysical Tests of Chiral Effective Field Theory at Supranuclear Densities
• Formation of Massive Black Holes in Galactic Nuclei: Runaway Tidal Encounters
• A geometric approach to the precession of compact binaries
• Effective field theory methods to model compact binaries
• Do electron-capture supernovae make neutron stars? First multidimensional hydrodynamic simulations of the oxygen deflagration
• Probing the existence of ultralight bosons with a single gravitational-wave measurement
• Searches for Continuous-Wave Gravitational Radiation
• Spin Evolution of Stellar-mass Black Hole Binaries in Active Galactic Nuclei
• Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements
• Transient resonances in the inspirals of point particles into black holes
• Relativistic models of magnetars: the twisted-torus magnetic field configuration
• Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry
• Constraints on the astrophysical environment of binaries with gravitational-wave observations
• Gravitational waves from bubble dynamics: Beyond the Envelope
• Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case
• Absorption Effects due to Spin in the Worldline Approach to Black Hole Dynamics
• Accelerated gravitational-wave parameter estimation with reduced order modeling
• A Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background
• Accurate numerical simulations of inspiralling binary neutron stars and their comparison with effective-one-body analytical models
• Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies
• Unveiling the first black holes with JWST: multi-wavelength spectral predictions
• Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
• Binary Black Holes: Spin Dynamics and Gravitational Recoil
• Evolution of Einstein-scalar-Gauss-Bonnet gravity using a modified harmonic formulation
• Gravitational self-force on generic bound geodesics in Kerr spacetime
• Supernova Neutrino Burst Detection with the Deep Underground Neutrino Experiment
• A magnetar engine for short GRBs and kilonovae
• A Triple Origin for the Heavy and Low-Spin Binary Black Holes Detected by LIGO/Virgo
• Coherent network analysis technique for discriminating gravitational-wave bursts from instrumental noise
• Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants
• Detection of stellar light from quasar host galaxies at redshifts above 6
• Anisotropy of the astrophysical gravitational wave background: analytic expression of the angular power spectrum and correlation with cosmological observations
• Magnetically driven winds from differentially rotating neutron stars and X-ray afterglows of short gamma-ray bursts
• Quasiuniversal properties of neutron star mergers
• QCD-induced Electroweak Phase Transition
• Can a supernova be located by its neutrinos?
• High redshift radio galaxies and divergence from the CMB dipole
• Energy and periastron advance of compact binaries on circular orbits at the fourth post-Newtonian order
• Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae
• Friction pressure on relativistic bubble walls
• Finding the chiral gravitational wave background of an axion-SU(2) inflationary model using CMB observations and laser interferometers
• Tidal Love numbers of a slowly spinning neutron star
• Anisotropies and non-Gaussianity of the Cosmological Gravitational Wave Background
• Ambiguity-Free Completion of the Equations of Motion of Compact Binary Systems at the Fourth Post-Newtonian Order
• Three-dimensional core-collapse supernova simulations of massive and rotating progenitors
• One-armed Spiral Instability in a Low T/|W| Postbounce Supernova Core
• Accuracy of inference on the physics of binary evolution from gravitational-wave observations
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
• Effective potentials and morphological transitions for binary black-hole spin precession
• Well-posed formulation of Lovelock and Horndeski theories
• Gravitational waves from black hole-neutron star binaries I: Classification of waveforms
• Short GRB Host Galaxies I: Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets
• Compact binary systems in scalar-tensor gravity. II. Tensor gravitational waves to second post-Newtonian order
• Gravitational-wave energy flux for compact binaries through second order in the mass ratio
• On the capture of dark matter by neutron stars
• Inferring the post-merger gravitational wave emission from binary neutron star coalescences
• The self-consistent gravitational self-force
• PPN Parameter $\gamma$ and Solar System Constraints of Massive Brans-Dicke Theories
• Primordial Black Holes as Dark Matter: Almost All or Almost Nothing
• An astrometric search method for individually resolvable gravitational wave sources with Gaia
• Polarizations of gravitational waves in $f(R)$ gravity
• Bubble wall velocity: heavy physics effects
• A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
• Effects of hyperons in binary neutron star mergers
• Gravitational waves from nonspinning black hole-neutron star binaries: dependence on equations of state
• Unifying the Zoo of Jet-Driven Stellar Explosions
• Sixth post-Newtonian nonlocal-in-time dynamics of binary systems
• Gravitational Waves from a Particle in Circular Orbits around a Schwarzschild Black Hole to the 22nd Post-Newtonian Order
• Constraining the masses of microlensing black holes and the mass gap with Gaia DR2
• Relativistic magnetohydrodynamics in dynamical spacetimes: A new AMR implementation
• Failed Supernovae Explain the Compact Remnant Mass Function
• Gravitational Waves from Collapsing Domain Walls
• GW150914: Spin based constraints on the merger time of the progenitor system
• Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signals
• Constraining nuclear equations of state using gravitational waves from hypermassive neutron stars
• Gravitational radiation from a bulk flow model
• Hierarchical Black-Hole Mergers in Multiple Systems: Constrain the Formation of GW190412, GW190814 and GW190521-like events
• On the likelihood of detecting gravitational waves from Population III compact object binaries
• Filtered Dark Matter at a First Order Phase Transition
• Comparisons of eccentric binary black hole simulations with post-Newtonian models
• Energy and angular momentum flow into a black hole in a binary
• Metallicity-constrained merger rates of binary black holes and the stochastic gravitational wave background
• Probing the scale of grand unification with gravitational waves
• Cubic order spin effects in the dynamics and gravitational wave energy flux of compact object binaries
• Distinguishing Primordial Black Holes from Astrophysical Black Holes by Einstein Telescope and Cosmic Explorer
• Research Note: The Expected Spins of Gravitational Wave Sources With Isolated Field Binary Progenitors
• Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings
• Simulations of non-equal mass black hole binaries with spectral methods
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. VIII. A Comparison to Cosmological Short-duration Gamma-ray Bursts
• Gravitational wave echoes through new windows
• Axion Inflation with an SU(2) Gauge Field: Detectable Chiral Gravity Waves
• Gravitational waveforms from a point particle orbiting a Schwarzschild black hole
• Orbital Dynamics of Binary Boson Star Systems
• Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift
• A New Multi-Energy Neutrino Radiation-Hydrodynamics Code in Full General Relativity and Its Application to Gravitational Collapse of Massive Stars
• Anisotropies of Gravitational Wave Backgrounds: A Line Of Sight Approach
• Gravitational Waves from First-Order Phase Transitions: LIGO as a Window to Unexplored Seesaw Scales
• Star formation at the smallest scales; A JWST study of the clump populations in SMACS0723
• Joint constraints on the field-cluster mixing fraction, common envelope efficiency, and globular cluster radii from a population of binary hole mergers via deep learning
• Masses and Luminosities of O and B - type stars and red super giants
• Spectral sirens: cosmology from the full mass distribution of compact binaries
• The Clustering Evolution of Primordial Black Holes
• A High Braking Index for a Pulsar
• Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
• The origin of the first neutron star -- neutron star merger
• Post-Newtonian accurate parametric solution to the dynamics of spinning compact binaries in eccentric orbits: The leading order spin-orbit interaction
• The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse
• Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution
• Black hole-neutron star binary merger: Dependence on black hole spin orientation and equations of state
• The evolution of black-hole mass and angular momentum
• An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• The Rise of the First Stars: Supersonic Streaming, Radiative Feedback, and 21-cm Cosmology
• Numerical relativity simulation of GW150914 in Einstein dilaton Gauss-Bonnet gravity
• Slowly rotating neutron stars in scalar-tensor theories with a massive scalar field
• Neutrino signature of supernova hydrodynamical instabilities in three dimensions
• Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
• High-Energy Neutrino Emission from Short Gamma-Ray Bursts: Prospects for Coincident Detection with Gravitational Waves
• Is black-hole ringdown a memory of its progenitor?
• The Spatial Clustering of Primordial Black Holes
• Testing massive star evolution, star-formation history and feedback at low metallicity : Spectroscopic analysis of OB stars in the SMC Wing
• Scaling from gauge and scalar radiation in Abelian Higgs string networks
• Perturbed Kerr Black Holes can probe deviations from General Relativity
• New twists in compact binary waveform modelling: a fast time domain model for precession
• Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies
• Generalized Uncertainty Principle, Black Holes, and White Dwarfs: A Tale of Two Infinities
• Numerical simulations of single and binary black holes in scalar-tensor theories: circumventing the no-hair theorem
• A comparison between star formation rate diagnostics and rate of core collapse supernovae within 11 Mpc
• The Search for Failed Supernovae with the Large Binocular Telescope: Constraints from 7 Years of Data
• Analysis of broad-lined Type Ic supernovae from the (intermediate) Palomar Transient Factory
• General-relativistic resistive-magnetohydrodynamic simulations of binary neutron stars
• Measuring the star formation rate with gravitational waves from binary black holes
• Cosmic Rulers
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields
• Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints
• Bayesian Evidence for Both Astrophysical and Primordial Black Holes: Mapping the GWTC-2 Catalog to Third-Generation Detectors
• The dynamics of the gravitational two-body problem at fourth post-Newtonian order and at quadratic order in the Newton constant
• Design and Sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
• General-relativistic precession in a black-hole binary
• Discriminating Strange Star Mergers from Neutron Star Mergers by Gravitational-Wave Measurements
• Cosmological Background Interpretation of Pulsar Timing Array Data
• Method for all-sky searches of continuous gravitational wave signals using the frequency-Hough transform
• Phasing of gravitational waves from inspiralling eccentric binaries at the third-and-a-half post-Newtonian order
• SpECTRE: A Task-based Discontinuous Galerkin Code for Relativistic Astrophysics
• Exploring the sensitivity of gravitational wave detectors to neutron star physics
• Color Unifed Dynamical Axion
• Probing Anisotropies of the Stochastic Gravitational Wave Background with LISA
• Disks, spikes, and clouds: distinguishing environmental effects on BBH gravitational waveforms
• Unified treatment of cosmological perturbations from super-horizon to small scales
• Non-linear statistics of primordial black holes from gaussian curvature perturbations
• Well-posedness of formulations of the Einstein equations with dynamical lapse and shift conditions
• Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters
• Polluting the pair-instability mass gap for binary black holes through super-Eddington accretion in isolated binaries
• Frequency and time domain inspiral templates for comparable mass compact binaries in eccentric orbits
• Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
• How to observe a non-Kerr spacetime
• Invariant quantities in the scalar-tensor theories of gravitation
• A Note on the evolution of cosmic string/superstring networks
• Satellite Dwarf Galaxies in a Hierarchical Universe: The Prevalence of Dwarf-Dwarf Major Mergers
• High Resolution Calculations of Merging Neutron Stars I: Model Description and Hydrodynamic Evolution
• First-post-Newtonian quadrupole tidal interactions in binary systems
• Pushing 1D CCSNe to explosions: model and SN 1987A
• Foundations of an effective-one-body model for coalescing binaries on eccentric orbits
• Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta
• Maximum Black Hole mass across Cosmic Time
• Real-Time Detection of Gravitational Waves from Binary Neutron Stars using Artificial Neural Networks
• Mu- and Tau-Neutrino Spectra Formation in Supernovae
• Measuring a Parity Violation Signature in the Early Universe via Ground-based Laser Interferometers
• Gravitational waves from three-dimensional core-collapse supernova models: The impact of moderate progenitor rotation
• Probing Fundamental Physics with Gravitational Waves: The Next Generation
• Electroweak baryogenesis at high wall velocities
• Gravitational Wave Signatures from Low-mode Spiral Instabilities in Rapidly Rotating Supernova Cores
• Measuring the dark matter environments of black hole binaries with gravitational waves
• Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap
• Strong-Field Scattering of Two Black Holes: Numerics Versus Analytics
• Binary Neutron Stars with Generic Spin, Eccentricity, Mass ratio, and Compactness - Quasi-equilibrium Sequences and First Evolutions
• Interplay of Neutrino Opacities in Core-collapse Supernova Simulations
• Limits on intermediate-mass black holes in six Galactic globular clusters with integral-field spectroscopy
• Effective Field Theory and Decoupling in Multi-field Inflation: An Illustrative Case Study
• Dynamical descalarization in binary black hole mergers
• Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
• Gravitational Waves from Broken Cosmic Strings: The Bursts and the Beads
• Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
• The First Billion Years project: birthplaces of direct collapse black holes
• Constraints on quasi-normal-mode frequencies with LIGO-Virgo binary-black-hole observations
• Accuracy Requirements for Empirically-Measured Selection Functions
• Are small radii of compact stars ruled out by GW170817/AT2017gfo?
• Primordial Black Hole Dark Matter and the LIGO/Virgo observations
• The Black Hole Mass Function from Gravitational Wave Measurements
• Formation pathway of Population III coalescing binary black holes through stable mass transfer
• Modeling the gravitational wave signature of neutron star black hole coalescences: PhenomNSBH
• Ability of LIGO and LISA to probe the equation of state of the early Universe
• Duality Cascade in Brane Inflation
• The Supercooled Universe
• Perturbations of Schwarzschild black holes in the Lorenz gauge: Formulation and numerical implementation
• The cosmic merger rate density evolution of compact binaries formed in young star clusters and in isolated binaries
• Beyond second-order convergence in simulations of magnetised binary neutron stars with realistic microphysics
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• Stochastic gravitational-wave background from metastable cosmic strings
• Improved methods for simulating nearly extremal binary black holes
• Repeated mergers and ejection of black holes within nuclear star clusters
• On the final fate of compact boson star mergers
• Parameterized Post-Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity
• Massive Black Hole Binaries from Collisional Runaways
• Detecting scalar fields with Extreme Mass Ratio Inspirals
• General relativistic simulations of black hole-neutron star mergers: Effects of magnetic fields
• Evolution of Mass Functions of Coeval Stars through Wind Mass Loss and Binary Interactions
• Bondi accretion in the early universe
• Influence of heavy modes on perturbations in multiple field inflation
• Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN
• General relativistic viscous hydrodynamics of differentially rotating neutron stars
• Towards a Realistic Explosion Landscape for Binary Population Synthesis
• Analysis of Galactic late-type O dwarfs: more constraints on the weak wind problem
• The influence of the distribution of cosmic star formation at different metallicities on the properties of merging double compact objects
• The Spin Distribution of Fast Spinning Neutron Stars in Low Mass X-Ray Binaries: Evidence for Two Sub-Populations
• Tidal deformability and I-Love-Q relations for gravastars with polytropic thin shells
• One-loop Gravitational Bremsstrahlung and Waveforms from a Heavy-Mass Effective Field Theory
• GLADE+: An Extended Galaxy Catalogue for Multimessenger Searches with Advanced Gravitational-wave Detectors
• Neutrino-driven Explosions
• The First Massive Black Hole Seeds and Their Hosts
• Search for Dark Matter Effects on Gravitational Signals from Neutron Star Mergers
• Neutron stars: new constraints on asymmetric dark matter
• Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order
• Compact binary systems in scalar-tensor gravity. III. Scalar waves and energy flux
• Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments
• Neural Importance Sampling for Rapid and Reliable Gravitational-Wave Inference
• Supernova rates from the SUDARE VST-Omegacam search. I
• General Relativistic Modeling of Magnetized Jets from Accreting Black Holes
• Are there any stable magnetic fields in barotropic stars?
• First predictions of the angular power spectrum of the astrophysical gravitational wave background
• Gravitational wave echoes from black hole area quantization
• Correlated Signatures of Gravitational-Wave and Neutrino Emission in Three-Dimensional General-Relativistic Core-Collapse Supernova Simulations
• Probing the Universe through the Stochastic Gravitational Wave Background
• Super-Eddington Accretion and Feedback from the First Massive Seed Black Holes
• Reducing orbital eccentricity of precessing black-hole binaries
• Accounting for Source Uncertainties in Analyses of Astronomical Survey Data
• Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the first order in rotation
• Directed searches for gravitational waves from ultralight bosons
• A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations
• Numerical binary black hole collisions in dynamical Chern-Simons gravity
• Radiation-Reaction in the Effective Field Theory Approach to Post-Minkowskian Dynamics
• Turning in the landscape: a new mechanism for generating Primordial Black Holes
• Non-perturbative non-Gaussianity and primordial black holes
• Stochastic Gravitational-Wave Background from Binary Black Holes and Binary Neutron Stars and Implications for LISA
• Intermediate Mass Black Hole Formation in compact Young Massive Star Clusters
• Reducing eccentricity in black-hole binary evolutions with initial parameters from post-Newtonian inspiral
• Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity
• Ultralight boson cloud depletion in binary systems
• Gravitational wave signatures of ultralight vector bosons from black hole superradiance
• Standard sirens with a running Planck mass
• SN 2009bb: a Peculiar Broad-Lined Type Ic Supernova
• Estimation of the Sensitive Volume for Gravitational-wave Source Populations Using Weighted Monte Carlo Integration
• Characterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes
• Upper limits on the observational effects of nuclear pasta in neutron stars
• Inadequacies of the Fisher Information Matrix in gravitational-wave parameter estimation
• Black hole superradiant instability from ultralight spin-2 fields
• Symmetric nuclear matter from the strong interaction
• Primordial black holes as biased tracers
• Large Tensor Non-Gaussianity from Axion-Gauge Fields Dynamics
• Discovering intermediate-mass black hole lenses through gravitational wave lensing
• Primordial black holes from strong first-order phase transitions
• The powerful jet of an off-nuclear intermediate-mass black hole in the spiral galaxy NGC 2276
• Prospects for observing extreme-mass-ratio inspirals with LISA
• Merger rate density of Population III binary black holes below, above, and in the pair-instability mass gap
• The Cosmic Radio Dipole: Estimators and Frequency Dependence
• Exploring Evaporating Primordial Black Holes with Gravitational Waves
• The NewAthena mission concept in the context of the next decade of X-ray astronomy
• A non-interacting Galactic black hole candidate in a binary system with a main-sequence star
• Massive black hole merger rates: the effect of kpc separation wandering and supernova feedback
• Axion Gauge Field Inflation and Gravitational Leptogenesis: A Lower Bound on B Modes from the Matter-Antimatter Asymmetry of the Universe
• Gravitomagnetic resonant excitation of Rossby modes in coalescing neutron star binaries
• Second Order Gravitational Self-Force
• Signals in the tidal deformability for phase transitions in compact stars with constraints from GW170817
• kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter
• Signatures of non-gaussianity in the isocurvature modes of primordial black hole dark matter
• Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions
• Towards adiabatic waveforms for inspiral into Kerr black holes: II. Dynamical sources and generic orbits
• Gravitational waves in Einstein-æther and generalized TeVeS theory after GW170817
• Logarithmic Duality of the Curvature Perturbation
• Predicting the binary black hole population of the Milky Way with cosmological simulations
• Distinguishing compact binary population synthesis models using gravitational-wave observations of coalescing binary black holes
• Continuous gravitational waves from neutron stars: current status and prospects
• Multiband gravitational-wave event rates and stellar physics
• Observational signatures of microlensing in gravitational waves at LIGO/Virgo frequencies
• EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\gtrsim 6$
• Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits
• Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
• Low Mass Black Holes from Dark Core Collapse
• The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region
• Gravitational waves from inspiralling compact binaries: hexagonal template placement and its efficiency in detecting physical signals
• A non-local theory of massive gravity
• How loud are neutron star mergers?
• Environmental Effects for Gravitational-wave Astrophysics
• Eccentric binary neutron star mergers
• Mixing of spherical and spheroidal modes in perturbed Kerr black holes
• All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data
• Derivation of local-in-time fourth post-Newtonian ADM Hamiltonian for spinless compact binaries
• How does a dark compact object ringdown?
• The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin
• Characterizing the Cosmological Gravitational Wave Background Anisotropies and non-Gaussianity
• Projected Constraints on Scalarization with Gravitational Waves from Neutron Star Binaries
• Black hole formation from a general quadratic action for inflationary primordial fluctuations
• Constraining the abundance of primordial black holes with gravitational lensing of gravitational waves at LIGO frequencies
• Axial perturbations of the scalarized Einstein-Gauss-Bonnet black holes
• Intermediate-mass Black Holes from High Massive-star Binary Fractions in Young Star Clusters
• Gravitational Self-force in a Radiation Gauge
• Gravitational-wave signal of a core-collapse supernova explosion of a 15 Solar mass star
• Global Description of Beta Decay with the Axially-Deformed Skyrme Finite Amplitude Method: Extension to Odd-Mass and Odd-Odd Nuclei
• Tidal heating as a discriminator for horizons in extreme mass ratio inspirals
• The disappearance of the helium-giant progenitor of the type Ib supernova iPTF13bvn and constraints on its companion
• Multipole Love Relations
• Multi-band gravitational-wave astronomy: parameter estimation and tests of general relativity with space and ground-based detectors
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Inferring supernova IIb/Ib/Ic ejecta properties from light curves and spectra: Correlations from radiative-transfer models
• A first search for a stochastic gravitational-wave background from ultralight bosons
• Can we measure individual black-hole spins from gravitational-wave observations?
• Simulating merging binary black holes with nearly extremal spins
• Kadath: a spectral solver for theoretical physics
• The low-end of the black hole mass function at cosmic dawn
• The LSC Glitch Group : Monitoring Noise Transients during the fifth LIGO Science Run
• Fingerprints of binary black hole formation channels encoded in the mass and spin of merger remnants
• Coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysis
• The most ordinary formation of the most unusual double black hole merger
• Effect of lensing magnification on the apparent distribution of black hole mergers
• Gravitational wave signatures in black-hole-forming core collapse
• Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817
• Black Hole Mergers From Globular Clusters Observable by LISA II: Resolved Eccentric Sources and the Gravitational Wave Background
• Abundance of primordial black holes with local non-Gaussianity in peak theory
• Magnetorotational core collapse of possible GRB progenitors. III. Three-dimensional models
• Dimensional regularization of local singularities in the 4th post-Newtonian two-point-mass Hamiltonian
• Correlation function of high-threshold regions and application to the initial small-scale clustering of primordial black holes
• Heavy Baryons in Compact Stars
• Extreme Mass-Ratio Inspirals in the Effective-One-Body Approach: Quasi-Circular, Equatorial Orbits around a Spinning Black Hole
• A targeted coherent search for gravitational waves from compact binary coalescences
• The Mock LISA Data Challenges: from Challenge 1B to Challenge 3
• Anisotropies in the stochastic gravitational-wave background: Formalism and the cosmic string case
• Observing Invisible Axions with Gravitational Waves
• Higgsed Chromo-Natural Inflation
• Is GW190521 the merger of black holes from the first stellar generations?
• Fast-moving stars around an intermediate-mass black hole in Omega Centauri
• Electromagnetic emission from axionic clouds and the quenching of superradiant instabilities
• Gravitational wave probes of dark matter: challenges and opportunities
• On the GBM event seen 0.4 sec after GW 150914
• AT2017gfo: Bayesian inference and model selection of multi-component kilonovae and constraints on the neutron star equation of state
• Searching for black hole echoes from the LIGO-Virgo Catalog GWTC-1
• Phases of dense matter in compact stars
• The Fate of Neutron Star Binary Mergers
• The `Red Supergiant Problem': the upper luminosity boundary of type-II supernova progenitors
• Supernova pointing with low- and high-energy neutrino detectors
• Thanks for the memory: measuring gravitational-wave memory in the first LIGO/Virgo gravitational-wave transient catalog
• Black Hole-Neutron Star Mergers with a Hot Nuclear Equation of State: Outflow and Neutrino-Cooled Disk for a Low-Mass, High-Spin Case
• Initial data for black hole-neutron star binaries: a flexible, high-accuracy spectral method
• Post-Newtonian dynamics and black hole thermodynamics in Einstein-scalar-Gauss-Bonnet gravity
• Gravitational waveforms in scalar-tensor gravity at 2PN relative order
• Prospects for gravitational-wave observations of neutron-star tidal disruption in neutron-star/black-hole binaries
• Reduced basis catalogs for gravitational wave templates
• Binary Neutron Star Mergers and Third Generation Detectors: Localization and Early Warning
• qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients
• All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
• Direct limits for scalar field dark matter from a gravitational-wave detector
• Testing Chern-Simons Modified Gravity with Gravitational-Wave Detections of Extreme-Mass-Ratio Binaries
• Primordial Gravitational Waves in Nonstandard Cosmologies
• When did Population III star formation end?
• Metallicity-dependent wind parameter predictions for OB stars
• Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
• Lunar Gravitational-Wave Antenna
• Correlated magnetic noise in global networks of gravitational-wave interferometers: observations and implications
• Turbulent Cold Flows Gave Birth to the First Quasars
• The Equation of State for the Nucleonic and Hyperonic Core of Neutron Stars
• SNEWS 2.0: A Next-Generation SuperNova Early Warning System for Multi-messenger Astronomy
• Distinguishing fuzzballs from black holes through their multipolar structure
• On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
• Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M supernova model
• Bayesian reconstruction of gravitational wave burst signals from simulations of rotating stellar core collapse and bounce
• Formation of massive seed black holes via collisions and accretion
• Linear mode stability of Kerr-Newman and its quasinormal modes
• New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter
• Gravitational Waves from Domain Walls in Pulsar Timing Array Datasets
• Optical pulsations from a transitional millisecond pulsar
• Dynamical Excision Boundaries in Spectral Evolutions of Binary Black Hole Spacetimes
• A new gravitational wave generation algorithm for particle perturbations of the Kerr spacetime
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Mergers of Magnetized Neutron Stars with Spinning Black Holes: Disruption, Accretion and Fallback
• Explaining LIGO's observations via isolated binary evolution with natal kicks
• Post-Newtonian Gravitational and Scalar Waves in Scalar-Gauss-Bonnet Gravity
• Spiral-wave wind for the blue kilonova
• Correlating features in the primordial spectra
• Parameter estimation with gravitational waves
• Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae
• Highly eccentric inspirals into a black hole
• Parameter estimation for heavy binary-black holes with networks of second-generation gravitational-wave detectors
• Center-of-Mass Equations of Motion and Conserved Integrals of Compact Binary Systems at the Fourth Post-Newtonian Order
• The influence of streaming velocities and Lyman-Werner radiation on the formation of the first stars
• All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data
• Constraints on ultralight scalar bosons within black hole spin measurements from LIGO-Virgo's GWTC-2
• Image-based deep learning for classification of noise transients in gravitational wave detectors
• Parameter estimation for binary black holes with networks of third generation gravitational-wave detectors
• On the nature of the 'hostless' short GRBs
• SN2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova
• Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
• Measuring the Angular Momentum Distribution in Core-Collapse Supernova Progenitors with Gravitational Waves
• Superfluidity and Superconductivity in Neutron Stars
• Holographic quark matter and neutron stars
• On the Deconfinement Phase Transition in Neutron-Star Mergers
• Model-independent inference on compact-binary observations
• Effective-one-body waveforms for precessing coalescing compact binaries with post-newtonian Twist
• The scaling density of axion strings
• Massive star evolution in close binaries:conditions for homogeneous chemical evolution
• Surrogate model for an aligned-spin effective one body waveform model of binary neutron star inspirals using Gaussian process regression
• Computing inspirals in Kerr in the adiabatic regime. I. The scalar case
• An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole
• Cosmology of axion dark matter
• A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations
• Towards asteroseismology of core-collapse supernovae with gravitational-wave observations - II. Spacetime perturbations
• Measurement of Parity Violation in the Early Universe using Gravitational-wave Detectors
• A Multipolar Effective One Body Model for Non-Spinning Black Hole Binaries
• From amplitudes to gravitational radiation with cubic interactions and tidal effects
• Cosmology and dark energy from joint gravitational wave-GRB observations
• Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
• Long-term dynamics of cosmological axion strings
• Potential gravitational-wave signatures of quantum gravity
• Reduced-order modeling with artificial neurons for gravitational-wave inference
• Discovery of the afterglow and host galaxy of the low redshift short GRB 080905A
• Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger
• Modelling the spectra of the kilonova AT2017gfo -- I: The photospheric epochs
• Hidden Markov model tracking of continuous gravitational waves from a neutron star with wandering spin
• Probing Dynamical Gravity with the Polarization of Continuous Gravitational Waves
• Repeated mergers, mass-gap black holes, and formation of intermediate-mass black holes in nuclear star clusters
• Gravitational ringing of rotating black holes in higher-derivative gravity
• On the Apparent Ambiguities in the Post-Newtonian Expansion for Binary Systems
• Explosions Driven by the Coalescence of a Compact Object with the Core of a Massive-Star Companion Inside a Common Envelope: Circumstellar Properties, Light Curves, and Population Statistics
• Dynamic Signatures of Black Hole Binaries with Superradiant Clouds
• The fifth-order post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach: potential contributions
• Probing Primordial Features with the Stochastic Gravitational Wave Background
• Gravitational-Wave Asteroseismology with Fundamental Modes from Compact Binary Inspirals
• A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation
• Improved Dynamical Constraints on the Mass of the central Black Hole in NGC 404
• Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity
• Spectroscopy of binary black hole ringdown using overtones and angular modes
• Reconstructing the calibrated strain signal in the Advanced LIGO detectors
• Numerical simulations of gravitational collapse in Einstein-aether theory
• Quasinormal modes of slowly-rotating black holes in dynamical Chern-Simons gravity
• Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
• Late Inspiral and Merger of Binary Black Holes in Scalar-Tensor Theories of Gravity
• Gravitational Self-Force Correction to the Innermost Stable Circular Equatorial Orbit of a Kerr Black Hole
• Proto-neutron stars with heavy baryons and universal relations
• Extra-Large Remnant Recoil Velocities and Spins from Near-Extremal-Bowen-York-Spin Black-Hole Binaries
• LISA data analysis: Source identification and subtraction
• Gravitational waves from bubble collisions and fluid motion in strongly supercooled phase transitions
• Detectability of Intermediate-Mass Black Holes in Multiband Gravitational Wave Astronomy
• Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions
• Black hole perturbation theory and gravitational self-force
• A First Targeted Search for Gravitational-Wave Bursts from Core-Collapse Supernovae in Data of First-Generation Laser Interferometer Detectors
• Supermassive Star Formation via Super Competitive Accretion in Slightly Metal-enriched Clouds
• Classical gravitational spinning-spinless scattering at $\mathcal{O}(G^2{S}^{\infty })$
• The Emergence of Structure in the Binary Black Hole Mass Distribution
• Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits
• Cover Your Basis: Comprehensive Data-Driven Characterization of the Binary Black Hole Population
• Effective-one-body waveforms from dynamical captures in black hole binaries
• Sharp Signals of Boson Clouds in Black Hole Binary Inspirals
• Energy versus Angular Momentum in Black Hole Binaries
• An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations
• Non-conservative effects on Spinning Black Holes from World-Line Effective Field Theory
• Black Hole Mergers from Hierarchical Triples in Dense Star Clusters
• Gravitational waves from remnant massive neutron stars of binary neutron star merger: Viscous hydrodynamics effects
• On the gravitational polarizability of black holes
• A Detailed Examination of Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of ${}^{208}$Pb with Minimal Modeling Assumptions
• Fourth post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach
• Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo
• The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae
• Precessional dynamics of black hole triples: binary mergers with near-zero effective spin
• Long gravitational-wave transients and associated detection strategies for a network of terrestrial interferometers
• Nonlinear gravitational self-force: second-order equation of motion
• Beta equilibrium in neutron star mergers
• Peccei-Quinn Phase Transition at LIGO
• The stability of toroidal fields in stars
• A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
• Merger rate of black hole binaries from globular clusters: theoretical error bars and comparison to gravitational wave data from GWTC-2
• Analytical model for gravitational-wave echoes from spinning remnants
• Primordial Black Holes from the QCD axion
• Efficient asymptotic frame selection for binary black hole spacetimes using asymptotic radiation
• Fast Neutrino Flavor Conversion in Core-Collapse Supernovae: A Parametric Study in 1D Models
• Black hole-neutron star mergers from triples
• The Sensitivity of Core-Collapse Supernovae to Nuclear Electron Capture
• Inferring the properties of a population of compact binaries in presence of selection effects
• Coherent Network Detection of Gravitational Waves: The Redundancy Veto
• Gravitational Waves from Global Cosmic Strings and Cosmic Archaeology
• Black Hole Dynamics in Einstein-Maxwell-Dilaton Theory
• Constraint damping of the conformal and covariant formulation of the Z4 system in simulations of binary neutron stars
• Bounding the Time Delay between High-energy Neutrinos and Gravitational-wave Transients from Gamma-ray Bursts
• Detecting gravitational waves from mountains on neutron stars in the Advanced Detector Era
• Regularization of fields for self-force problems in curved spacetime: foundations and a time-domain application
• Gravitational Wave and CMB Probes of Axion Kination
• PBH formation from spherically symmetric hydrodynamical perturbations: a review
• Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity
• New CMB constraints for Abelian Higgs cosmic strings
• The adiabatic evolution of orbital parameters in the Kerr spacetime
• Fast time variations of supernova neutrino fluxes and their detectability
• Polarization-based Tests of Gravity with the Stochastic Gravitational-Wave Background
• Search for ultralight bosons in Cygnus X-1 with Advanced LIGO
• On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism
• Metric perturbations produced by eccentric equatorial orbits around a Kerr black hole
• Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection
• Towards asteroseismology of core-collapse supernovae with gravitational-wave observations - I. Cowling approximation
• Bubble wall velocities in local equilibrium
• Spectropolarimetry of superluminous supernovae: insight into their geometry
• Equation of state effects in the core collapse of a $20$-$M_{\odot }$ star
• Gravitational Wave Anisotropies from Primordial Black Holes
• Determining the progenitors of merging black-hole binaries
• Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties
• Analytical high-order post-Newtonian expansions for extreme mass ratio binaries
• Primordial Black Holes from Supercooled Phase Transitions
• Polarization analysis of gravitational-wave backgrounds from the correlation signals of ground-based interferometers: measuring a circular-polarization mode
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal
• Studying strong phase transitions in neutron stars with gravitational waves
• Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• Formation sites of Population III star formation: The effects of different levels of rotation and turbulence on the fragmentation behavior of primordial gas
• Primordial black holes from long-range scalar forces and scalar radiative cooling
• Supernova Fallback as Origin of Neutron Star Spins and Spin-kick Alignment
• Evidence for a minimum ellipticity in millisecond pulsars
• Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
• The Initial Value Formulation of Dynamical Chern-Simons Gravity
• Probing multiple populations of compact binaries with third-generation gravitational-wave detectors
• Modeling multipolar gravitational-wave emission from small mass-ratio mergers
• Evolution of String-Wall Networks and Axionic Domain Wall Problem
• Classification methods for noise transients in advanced gravitational-wave detectors
• A Cool and Inflated Progenitor Candidate for the Type Ib Supernova 2019yvr at 2.6 Years Before Explosion
• THESEUS: a key space mission concept for Multi-Messenger Astrophysics
• IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes
• Extracting linear and nonlinear quasinormal modes from black hole merger simulations
• No massive black holes in the Milky Way halo
• The Hydrodynamic Origin of Neutron Star Kicks
• Neutrino Emission from Supernovae
• The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown
• Eccentric Black Hole-Neutron Star Mergers
• Anisotropies in the astrophysical gravitational-wave background: Predictions for the detection of compact binaries by LIGO and Virgo
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
• Conservative, gravitational self-force for a particle in circular orbit around a Schwarzschild black hole in a Radiation Gauge
• Resonant Tidal Excitation of Oscillation Modes in Merging Binary Neutron Stars: Inertial-Gravity Modes
• Binary Black Hole Mergers from Globular Clusters: the Impact of Globular Cluster Properties
• Well-posed formulation of scalar-tensor effective field theory
• Population III Binary Black Holes: Effects of Convective Overshooting on Formation of GW190521
• Constraints on Einstein-dilaton-Gauss-Bonnet gravity from Black Hole-Neutron Star Gravitational Wave Events
• Dynamics of compact binary systems in scalar-tensor theories: I. Equations of motion to the third post-Newtonian order
• A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity
• Short GRB Host Galaxies. II. A Legacy Sample of Redshifts, Stellar Population Properties, and Implications for their Neutron Star Merger Origins
• Relativistic description of dense matter equation of state and compatibility with neutron star observables: a Bayesian approach
• Pulsar Birthrate from Parkes Multi-beam Survey
• Neutron star mergers as a probe of modifications of general relativity with finite-range scalar forces
• Baryogenesis from a dark first-order phase transition
• Baryogenesis and gravity waves from a UV-completed electroweak phase transition
• Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
• Searching for Dark Matter with Neutron Star Mergers and Quiet Kilonovae
• Radiation-reaction force and multipolar waveforms for eccentric, spin-aligned binaries in the effective-one-body formalism
• Effective one body Hamiltonian of two spinning black-holes with next-to-next-to-leading order spin-orbit coupling
• The rapid growth phase of supermassive black holes
• Orbital fingerprints of ultralight scalar fields around black holes
• Disentangling Coalescing Neutron Star-White Dwarf Binaries for LISA
• Gravitational waves from 3D MHD core collapse simulations
• Tests of General Relativity with Gravitational-Wave Observations using a Flexible--Theory-Independent Method
• Analytical template for gravitational-wave echoes: signal characterization and prospects of detection with current and future interferometers
• Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation
• JWST-JADES. Possible Population III signatures at z=10.6 in the halo of GN-z11
• Inferring the core-collapse supernova explosion mechanism with gravitational waves
• Massive Stellar Triples Leading to Sequential Binary Black-Hole Mergers in the Field
• A New Window into Black Holes
• Energetics and phasing of nonprecessing spinning coalescing black hole binaries
• Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing run
• Toroidal Magnetic Fields in Type II Superconducting Neutron Stars
• Energy Transfer in Multi Field Inflation and Cosmological Perturbations
• Dynamics of black hole - neutron star binaries in young star clusters
• Spin-Orbit Misalignment of Merging Black-Hole Binaries with Tertiary Companions
• Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
• Field-theoretic derivation of bubble-wall force
• A new public code for initial data of unequal-mass, spinning compact-object binaries
• The importance of magnetic fields for the initial mass function of the first stars
• Gravitational self-force on a particle orbiting a Kerr black hole
• A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey
• Probing Dark Low-mass Halos and Primordial Black Holes with Frequency-dependent Gravitational Lensing Dispersions of Gravitational Waves
• Dead or Alive? Long-term evolution of SN 2015bh (SNhunt275)
• Inferring Core-Collapse Supernova Physics with Gravitational Waves
• Small mass plunging into a Kerr black hole: Anatomy of the inspiral-merger-ringdown waveforms
• High-Energy Neutrinos from Millisecond Magnetars formed from the Merger of Binary Neutron Stars
• Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
• Implications from GW170817 for $\Delta$-isobar admixed hypernuclear compact stars
• Polarizations of Gravitational Waves in Horndeski Theory
• Neutron star properties in density-dependent relativistic Hartree-Fock theory
• A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity
• Fixing extensions to General Relativity in the non-linear regime
• Detection methods for non-Gaussian gravitational wave stochastic backgrounds
• Breakdown of Hawking Evaporation opens new Mass Window for Primordial Black Holes as Dark Matter Candidate
• Evidence for an intermediate-mass black hole in the globular cluster NGC 6624
• No peaks without valleys: The stable mass transfer channel for gravitational-wave sources in light of the neutron star-black hole mass gap
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• Bubble wall velocities in the Standard Model and beyond
• What is the nature of the HESS J1731-347 compact object?
• Metallicity of stars formed throughout the cosmic history based on the observational properties of star forming galaxies
• On the formation of the first quasars
• Quasi-normal modes of black holes in Horndeski gravity
• Ringing of rotating black holes in higher-derivative gravity
• Gravitational Waves from Binary Mergers of Sub-solar Mass Dark Black Holes
• Null infinity waveforms from extreme-mass-ratio inspirals in Kerr spacetime
• A new analytic representation of the ringdown waveform of coalescing spinning black hole binaries
• (Small) Resonant non-Gaussianities: Signatures of a Discrete Shift Symmetry in the Effective Field Theory of Inflation
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• The impact of common envelope development criteria on the formation of LIGO/Virgo sources
• Multi-Messenger Time Delays from Lensed Gravitational Waves
• General-relativistic neutrino-radiation magnetohydrodynamic simulation of seconds-long black hole-neutron star mergers
• Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
• Comprehensive study of mass ejection and nucleosynthesis in binary neutron star mergers leaving short-lived massive neutron stars
• Hyperbolic slicings of spacetime: singularity avoidance and gauge shocks
• Supernova Model Discrimination with Hyper-Kamiokande
• Gravitational self-force from radiation-gauge metric perturbations
• Influence of internal structure on the motion of test bodies in extreme mass ratio situations
• Observable signatures of enhanced axion emission from protoneutron stars
• Constraining bosonic asymmetric dark matter with neutron star mass-radius measurements
• Pions in hot dense matter and their astrophysical implications
• The effect of matter structure on the gravitational waveform
• Updated constraints on amplitude and tilt of the tensor primordial spectrum
• The stability of poloidal magnetic fields in rotating stars
• PhenomXO4a: a phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
• Loop corrections and graceful exit in string cosmology
• Gravitational Lensing of Gravitational Waves: Effect of Microlens Population in Lensing Galaxies
• Tidal effects in the gravitational-wave phase evolution of compact binary systems to next-to-next-to-leading post-Newtonian order
• SWIGLAL: Python and Octave interfaces to the LALSuite gravitational-wave data analysis libraries
• Masses of the Goldstone modes in the CFL phase of QCD at finite density
• Gravitational-Wave Phasing of Quasi-Circular Compact Binary Systems to the Fourth-and-a-Half post-Newtonian Order
• Gravitational wave background from Population III binary black holes consistent with cosmic reionization
• Gravitational floating orbits around hairy black holes
• The mass gap, the spin gap, and the origin of merging binary black holes
• Parametrized ringdown spin expansion coefficients: a data-analysis framework for black-hole spectroscopy with multiple events
• Gravitational radiation from inspiralling compact objects: Spin effects to fourth Post-Newtonian order
• Gravitational waves in scalar-tensor theory to one-and-a-half post-Newtonian order
• Non-local massive gravity
• Generation and propagation of nonlinear quasi-normal modes of a Schwarzschild black hole
• Neutrinos from Supernovae as a Trigger for Gravitational Wave Search
• The formation of low metallicity globular clusters in dwarf galaxy mergers
• Binary black holes population and cosmology in new lights: Signature of PISN mass and formation channel in GWTC-3
• Bayesian analysis of the crust-core transition with a compressible liquid-drop model
• Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole to the 11th Post-Newtonian Order
• Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements
• Black Holes and WIMPs: All or Nothing or Something Else
• Models of the Primordial Standard Clock
• Tidal heating and torquing of a Kerr black hole to next-to-leading order in the tidal coupling
• Explaining the most energetic supernovae with an inefficient jet-feedback mechanism
• Parameterized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method
• Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
• Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron star signals
• Causal gravitational waves as a probe of free streaming particles and the expansion of the Universe
• Formation of Binary Black Holes Similar to GW190521 with a Total Mass of $\sim 150M_{\odot }$ from Population III Binary Star Evolution
• Equation of state effects in black hole-neutron star mergers
• A 10,000-solar-mass black hole in the nucleus of a bulgeless dwarf galaxy
• New conformally flat initial data for spinning black holes
• Cosmological inference using only gravitational wave observations of binary neutron stars
• The rich complexity of 21-cm fluctuations produced by the first stars
• Star cluster formation in the most extreme environments: Insights from the HiPEEC survey
• Accreting Millisecond X-Ray Pulsars
• Singlets in Composite Higgs Models in light of the LHC di-photon searches
• Gravitational wave spectroscopy of binary neutron star merger remnants with mode stacking
• Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background
• Implications for the origin of short gamma-ray bursts from their observed positions around their host galaxies
• Correlated noise in networks of gravitational-wave detectors: subtraction and mitigation
• A GRB and Broad-lined Type Ic Supernova from a Single Central Engine
• R-modes in neutron stars: Theory and observations
• Extreme mass ratio inspirals with spinning secondary: a detailed study of equatorial circular motion
• The Birth Function for Black Holes and Neutron Stars in Close Binaries
• String Fragmentation in Supercooled Confinement and Implications for Dark Matter
• Gravitational-wave cutoff frequencies of tidally disruptive neutron star-black hole binary mergers
• Model-independent bubble wall velocities in local thermal equilibrium
• Spinning test-body orbiting around Schwarzschild black hole: circular dynamics and gravitational-wave fluxes
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Neutron star bulk viscosity, "spin-flip" and GW emission of newly born magnetars
• Constraints on the dense matter EOS from the measurements of PSR J0737-3039A moment of inertia and PSR J0751+1807 mass
• Critical collapse and the primordial black hole initial mass function
• Dynamical Friction in Gravitational Atoms
• Black-hole ringdown as a probe of higher-curvature gravity theories
• Resonant Tidal Excitations of Inertial Modes in Coalescing Neutron Star Binaries
• Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
• Neutrino transport in general relativistic neutron star merger simulations
• Polar quasinormal modes of the scalarized Einstein-Gauss-Bonnet black holes
• Damping of density oscillations in neutrino-transparent nuclear matter
• Black Hole Gravitational Waves in the Effective Field Theory of Gravity
• New Estimates of the Solar-Neighborhood Massive-Stars Birthrate and the Galactic Supernova Rate
• Gravitational wave asteroseismology with protoneutron stars
• The Dependence of the Neutrino Mechanism of Core-Collapse Supernovae on the Equation of State
• Mechanics of extended masses in general relativity
• Matter Neutrino Resonance Transitions above a Neutron Star Merger Remnant
• Wiggly Whipped Inflation
• Frequency-domain gravitational waveform models for inspiraling binary neutron stars
• Gravitational waves from f-modes excited by the inspiral of highly eccentric neutron star binaries
• Rush the inspiral: efficient Effective One Body time-domain gravitational waveforms
• Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning Compact Binaries to the Fourth Post-Newtonian Order
• Equation of state constraints from nuclear physics, neutron star masses, and future moment of inertia measurements
• Direct detection of gravitational waves can measure the time variation of the Planck mass
• Template-based Gravitational-Wave Echoes Search Using Bayesian Model Selection
• Nonlinear-in-spin effects in effective-one-body waveform models of spin-aligned, inspiralling, neutron star binaries
• Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries
• Standard Clock in Primordial Density Perturbations and Cosmic Microwave Background
• A practical, covariant puncture for second-order self-force calculations
• Monte-Carlo neutrino transport in neutron star merger simulations
• Gravitational wave parameter estimation with compressed likelihood evaluations
• R-axion at colliders
• GW$\times$LSS: Chasing the Progenitors of Merging Binary Black Holes
• The universal Teukolsky equations and black hole perturbations in higher-derivative gravity
• Detection and Classification of Supernova Gravitational Waves Signals: A Deep Learning Approach
• Systematics of prompt black-hole formation in neutron star mergers
• Highly Eccentric Kozai Mechanism and Gravitational-Wave Observation for Neutron Star Binaries
• Dimensional regularization of the IR divergences in the Fokker action of point-particle binaries at the fourth post-Newtonian order
• Effective-one-body waveforms for binary neutron stars using surrogate models
• Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the second order in rotation
• Nonlinear gravitational self-force. I. Field outside a small body
• Thermal properties of hot and dense matter with finite range interactions
• Jet Dynamics in Compact Object Mergers: GW170817 Likely had a Successful Jet
• Distinctive signatures of space-time diffeomorphism breaking in EFT of inflation
• How many supernovae are we missing at high redshift?
• High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers
• An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers
• The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology
• Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order
• Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations
• Whipped inflation
• Nonlinear studies of binary black hole mergers in Einstein-scalar-Gauss-Bonnet gravity
• Charged current neutrino interactions in hot and dense matter
• Gravitational radiation reaction and second order perturbation theory
• Formation of the first stars and black holes
• Primordial Black Holes from Cosmic Domain Walls
• Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs
• End-to-end kilonova models of neutron-star mergers with delayed black-hole formation
• Chemically Homogeneous Evolution: A rapid population synthesis approach
• Subtracting glitches from gravitational-wave detector data during the third observing run
• Trans-Ejecta High-Energy Neutrino Emission from Binary Neutron Star Mergers
• Production of very light elements and strontium in the early ejecta of neutron star mergers
• Fourier domain gravitational waveforms for precessing eccentric binaries
• Accelerating gravitational wave parameter estimation with multi-band template interpolation
• An extremely metal poor star complex in the reionization era: Approaching Population III stars with JWST
• Field theory simulation of Abelian-Higgs cosmic string cusps
• Numerical simulations of neutron star-black hole binaries in the near-equal-mass regime
• Evolution of small-mass-ratio binaries with a spinning secondary
• A hybrid post-Newtonian -- effective-one-body scheme for spin-precessing compact-binary waveforms
• Neutrino Emission as Diagnostics of Core-Collapse Supernovae
• Outlook for detecting the gravitational wave displacement and spin memory effects with current and future gravitational wave detectors
• Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective
• Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
• Breaking the spell of Gaussianity: forecasting with higher order Fisher matrices
• Jumping the gap: searching for LIGO's biggest black holes
• Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data
• A complete gauge-invariant formalism for arbitrary second-order perturbations of a Schwarzschild black hole
• Detecting Gravitational Waves in Data with Non-Gaussian Noise
• Measurement and subtraction of Schumann resonances at gravitational-wave interferometers
• Lattice Simulations of Axion-U(1) Inflation
• Massive stars in sub-parsec rings around galactic centers
• Intermediate-mass black holes in colliding clusters: Implications for lower-frequency gravitational-wave astronomy
• Constraints on Core Collapse from the Black Hole Mass Function
• Accelerating parameter estimation of gravitational waves from compact binary coalescence using adaptive frequency resolutions
• Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
• The Close Stellar Companions to Intermediate Mass Black Holes
• Thermal properties of supernova matter: The bulk homogeneous phase
• Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993
• Gravitational-Wave Constraints on an Effective Field-Theory Extension of General Relativity
• On the formation of GW190814
• Modeling the postmerger gravitational wave signal and extracting binary properties from future binary neutron star detections
• Emergence of Calabi-Yau manifolds in high-precision black hole scattering
• GeV emission from a compact binary merger
• Testing Brans-Dicke gravity using the Einstein telescope
• Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
• Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation
• Environmental Noise in Advanced LIGO Detectors
• Extreme mass-ratio inspirals around a spinning horizonless compact object
• Exploring Features in the Binary Black Hole Population
• Regularization parameters for the self force in Schwarzschild spacetime: II. gravitational and electromagnetic cases
• Third post-Newtonian gravitational waveforms for compact binary systems in general orbits: Instantaneous terms
• Apples and Oranges: Comparing black holes in X-ray binaries and gravitational-wave sources
• Fast Self-forced Inspirals
• Gravitational self-force on eccentric equatorial orbits around a Kerr black hole
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• Resolved [CII] Emission from z>6 Quasar Host -- Companion Galaxy Pairs
• Radiation reaction and the self-force for a point mass in general relativity
• A New Method to Observe Gravitational Waves emitted by Core Collapse Supernovae
• Gravitational waves from compact binaries in post-Newtonian accurate hyperbolic orbits
• Stochastic Gravitational Wave Background from Global Cosmic Strings
• Supernovae and their host galaxies. I. The SDSS DR8 database and statistics
• Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
• The Star Formation Rate Distribution Function of the Local Universe
• Gravitational waves from Population III binary black holes formed by dynamical capture
• Metric of a tidally distorted, nonrotating black hole
• Properties of the stochastic astrophysical gravitational wave background: astrophysical sources dependencies
• Peaks and primordial black holes: the effect of non-Gaussianity
• Supernova neutrinos and nucleosynthesis
• How effective is machine learning to detect long transient gravitational waves from neutron stars in a real search?
• $\text{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors
• Leptogenesis triggered by a first-order phase transition
• Drifting Oscillations in Axion Monodromy
• The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources
• Implications of the mass $M=2.17_{-0.10}^{+0.11}$M${}_{\odot }$ of PSR~J0740+6620 on the Equation of State of Super-Dense Neutron-Rich Nuclear Matter
• SN 2017ein and the Possible First Identification of a Type Ic Supernova Progenitor
• Measuring chiral gravitational waves in Chern-Simons gravity with CMB bispectra
• Biases in parameter estimation from overlapping gravitational-wave signals in the third generation detector era
• Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO--Virgo data
• Partial-envelope stripping and nuclear-timescale mass transfer from evolved supergiants at low metallicity
• Tidal Deformability of Dark Matter Admixed Neutron Stars
• Multi-messenger observations of binary neutron star mergers in the O4 run
• The search for failed supernovae with the Large Binocular Telescope: a new candidate and the failed SN fraction with 11 yr of data
• Coalescing black hole binaries from globular clusters: mass distributions and comparison to gravitational wave data from GWTC-3
• Time-dependence of the astrophysical stochastic gravitational wave background
• Star formation and nuclear activity in luminous infrared galaxies: An infrared through radio review
• Black Hole and Neutron Star Binary Mergers in Triple Systems: II. Merger Eccentricity and Spin-Orbit Misalignment
• Gravitational waves and kicks from the merger of unequal mass, highly compact boson stars
• Classification methods for noise transients in advanced gravitational-wave detectors II: performance tests on Advanced LIGO data
• Magnetars: a short review and some sparse considerations
• PBH formation from overdensities in delayed vacuum transitions
• Measuring the net circular polarization of the stochastic gravitational wave background with interferometers
• Nuclear Equation of state for Compact Stars and Supernovae
• Generalised tensor fluctuations and inflation
• Probing Models of Extended Gravity using Gravity Probe B and LARES experiments
• Prospects for probing gravitational waves from primordial black hole binaries
• On the Ambiguity in Relativistic Tidal Deformability
• Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
• Distance and properties of NGC 4993 as the host galaxy of a gravitational wave source, GW170817
• Optical measurement of superluminal motion in the neutron-star merger GW170817
• How to simulate global cosmic strings with large string tension
• The Population III origin of GW190521
• Cosmological dynamics and dark energy from non-local infrared modifications of gravity
• The form of cosmic string cusps
• Echoes from the Abyss: A highly spinning black hole remnant for the binary neutron star merger GW170817
• Minimal Length and Small Scale Structure of Spacetime
• Supercool Composite Dark Matter Beyond 100 TeV
• Probing the nature of central objects in extreme-mass-ratio inspirals with gravitational waves
• Hyperons in neutron stars and supernova cores
• Finite-temperature extension for cold neutron star equations of state
• Periastron advance in spinning black hole binaries: comparing effective-one-body and Numerical Relativity
• Primordial Black Holes from Broad Spectra: Abundance and Clustering
• The Minimum Testable Abundance of Primordial Black Holes at Future Gravitational-Wave Detectors
• Twin stars and the stiffness of the nuclear equation of state: ruling out strong phase transitions below $1.7n_0$ with the new NICER radius measurements
• The spin rate of pre-collapse stellar cores: wave-driven angular momentum transport in massive stars
• Cosmology and modified gravitational wave propagation from binary black hole population models
• The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis à vis One-Dimensional, Massive-star Supernova Progenitor Models
• Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare $r$-process Site
• A Parameter-Free Tour of the Binary Black Hole Population
• Next-to-leading tail-induced spin-orbit effects in the gravitational radiation flux of compact binaries
• Post-Newtonian spin-tidal couplings for compact binaries
• Hydrodynamic obstruction to bubble expansion
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
• Black Hole-Neutron Star Mergers in Globular Clusters
• Merging Black Holes in the Low-mass and High-mass Gaps from 2+2 Quadruple Systems
• Polarizations of Gravitational Waves in the Bumblebee Gravity Model
• Fingerprints of Primordial Universe Paradigms as Features in Density Perturbations
• Large amplitude behavior of the bulk viscosity of dense matter
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
• Gravitomagnetic response of an irrotational body to an applied tidal field
• Gravitational-wave data analysis using binary black-hole waveforms
• Self-Force Calculations with a Spinning Secondary
• Multi-mode black hole spectroscopy
• A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
• Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run
• Exploring tidal effects of coalescing binary neutron stars in numerical relativity II: Longterm simulations
• Neutron star crusts from mean field models constrained by chiral effective field theory
• Nitrogen enrichment and clustered star formation at the dawn of the Galaxy
• Implications of the low binary black hole aligned spins observed by LIGO
• The Effective Field Theory of Inflation Models with Sharp Features
• R-mode frequencies of slowly rotating relativistic neutron stars with realistic equations of state
• Adiabatic radiation reaction to the orbits in Kerr Spacetime
• Completion of metric reconstruction for a particle orbiting a Kerr black hole
• Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
• Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity
• Bubble Wall Velocity at Strong Coupling
• Heavy element nucleosynthesis in a collapsar
• Importance of transient resonances in extreme-mass-ratio inspirals
• Magnetar-powered superluminous supernovae must first be exploded by jets
• Growth of resonances and chaos for a spinning test particle in the Schwarzschild background
• The Transitional Stripped-Envelope SN 2008ax: Spectral Evolution and Evidence for Large Asphericity
• The Old Host-Galaxy Environment of SSS17a, the First Electromagnetic Counterpart to a Gravitational Wave Source
• Self-Force Calculations with Matched Expansions and Quasinormal Mode Sums
• Directed searches for continuous gravitational waves from binary systems: parameter-space metrics and optimal Scorpius X-1 sensitivity
• Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS
• The SPIRITS sample of Luminous Infrared Transients: Uncovering Hidden Supernovae and Dusty Stellar Outbursts in Nearby Galaxies
• Sub-radian-accuracy gravitational waves from coalescing binary neutron stars II: Systematic study on the equation of state, binary mass, and mass ratio
• Test for the Origin of Solar Mass Black Holes
• Gravitational-Wave Localization Alone Probes AGN Origin of Stellar-Mass Black Hole Mergers
• Detecting massive scalar fields with Extreme Mass-Ratio Inspirals
• Dynamics of compact binary systems in scalar-tensor theories: II. Center-of-mass and conserved quantities to 3PN order
• Early galaxy formation in warm dark matter cosmologies
• Host redshifts from gravitational-wave observations of binary neutron star mergers
• Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae
• A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• Gravitational waves with dark matter minispikes: the combined effect
• Localized correlated features in the CMB power spectrum and primordial bispectrum from a transient reduction in the speed of sound
• Spinning test-body orbiting around a Kerr black hole: circular dynamics and gravitational-wave fluxes
• Thermal Relics in Modified Cosmologies: Bounds on Evolution Histories of the Early Universe and Cosmological Boosts for PAMELA
• Accuracy and effectualness of closed-form, frequency-domain waveforms for non-spinning black hole binaries
• Constraining gravitational wave amplitude birefringence and Chern-Simons gravity with GWTC-2
• The Imprint of Relativistic Particles on the Anisotropies of the Stochastic Gravitational-Wave Background
• Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses
• Modified Dispersion Relation, Photon's Velocity, and Unruh Effect
• On the growth of massive scalar hair around a Schwarzschild black hole
• Birth, life, and death of black hole binaries around supermassive black holes: dynamical evolution of gravitational wave sources
• Numerical experiments with p F- and q D-strings: the formation of (p,q) bound states
• Cosmological bubble friction in local equilibrium
• Searching for photon-sector Lorentz violation using gravitational-wave detectors
• Tidal Love numbers of neutron stars in $f(R)$ gravity
• GWFish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks
• Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run
• Interplay between $\Delta$ Particles and Hyperons in Neutron Stars
• A fast and precise methodology to search for and analyse strongly lensed gravitational-wave events
• Gravitational Wave Signal for Quark Matter with Realistic Phase Transition
• m-Mode Regularization Scheme for the Self Force in Kerr Spacetime
• Cosmic Strings
• BSM with Cosmic Strings: Heavy, up to EeV mass, Unstable Particles
• Gravitational Waves from Neutrino Asymmetries in Core-Collapse Supernovae
• MLGWSC-1: The first Machine Learning Gravitational-Wave Search Mock Data Challenge
• Turbulence in Core-Collapse Supernovae
• Applying deep neural networks to the detection and space parameter estimation of compact binary coalescence with a network of gravitational wave detectors
• Merger rate density of binary black holes through isolated Population I, II, III and extremely metal-poor binary star evolution
• Modeling the horizon-absorbed gravitational flux for equatorial-circular orbits in Kerr spacetime
• The last migration trap of compact objects in AGN accretion disc
• Numerical relativity for D dimensional axially symmetric space-times: formalism and code tests
• Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
• Ain't No Mountain High Enough: Semi-Parametric Modeling of LIGO-Virgos Binary Black Hole Mass Distribution
• Statistical Gravitational Waveform Models: What to Simulate Next?
• Semi-analytic derivation of the threshold mass for prompt collapse in binary neutron star mergers
• First demonstration of early warning gravitational wave alerts
• Electron capture in stars
• The Metallicity Dependence of the Minimum Mass for Core-Collapse Supernovae
• Single-single gravitational-wave captures in globular clusters: Eccentric deci-Hertz sources observable by DECIGO and Tian-Qin
• Gravitational wave energy emission and detection rates of Primordial Black Hole hyperbolic encounters
• Constraints on Kerr-Newman black holes from merger-ringdown gravitational-wave observations
• Search for gravitational waves from the coalescence of sub-solar mass binaries in the first half of Advanced LIGO and Virgo's third observing run
• Revealing the formation of stellar-mass black hole binaries: The need for deci-Hertz gravitational wave observatories
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• Ultra-relativistic bubbles from the simplest Higgs portal and their cosmological consequences
• Core-collapse supernova simulations and the formation of neutron stars, hybrid stars, and black holes
• Constraining properties of the next nearby core-collapse supernova with multi-messenger signals
• Multiparameter tests of general relativity using multiband gravitational-wave observations
• Gravity and Scalar Fields
• Hybrid and quark star matter based on a non-perturbative equation of state
• Numerical solution of the 2+1 Teukolsky equation on a hyperboloidal and horizon penetrating foliation of Kerr and application to late-time decays
• Approach to scaling in axion string networks
• New Gogny interaction suitable for astrophysical applications
• The fifth-order post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach
• Code Comparison for Fast Flavor Instability Simulation
• Comprehensive numerical relativity -- effective-one-body comparison to inform improvements in waveform models for binary neutron star systems
• Teukolsky formalism for nonlinear Kerr perturbations
• Primordial Gravitational Wave Signals in Modified Cosmologies
• Parameter estimation for black hole echo signals and their statistical significance
• Search methods for continuous gravitational-wave signals from unknown sources in the advanced-detector era
• Ultralight dark matter detection with mechanical quantum sensors
• Simulations of PBH formation at the QCD epoch and comparison with the GWTC-3 catalog
• Self-force via $m$-mode regularization and 2+1D evolution: III. Gravitational field on Schwarzschild spacetime
• Spectral and morphological analysis of the remnant of Supernova 1987A with ALMA & ATCA
• Polarization test of gravitational waves from compact binary coalescences
• From core collapse to superluminous: The rates of massive stellar explosions from the Palomar Transient Factory
• Diffuse neutrino flux measurements with the Baikal-GVD neutrino telescope
• Illuminating the dark ages: Cosmic backgrounds from accretion onto primordial black hole dark matter
• Radiation reaction for spinning bodies in effective field theory II: Spin-spin effects
• An alternative interpretation of GW190412 as a binary black hole merger with a rapidly spinning secondary
• The effects of self-interacting bosonic dark matter on neutron star properties
• Spin-Precession: Breaking the Black Hole--Neutron Star Degeneracy
• Dark Matter or Regular Matter in Neutron Stars? How to tell the difference from the coalescence of compact objects
• Hamilton-Jacobi equation for spinning particles near black holes
• Self-consistent orbital evolution of a particle around a Schwarzschild black hole
• Dependence of Gravitational Wave Transient Rates on Cosmic Star Formation and Metallicity Evolution History
• Assessing the detectability of the secondary spin in extreme mass-ratio inspirals with fully-relativistic numerical waveforms
• Cosmological Phase Transition of Spontaneous Confinement
• Constraints on compact dark matter from gravitational wave microlensing
• Diversity of nuclear star cluster formation mechanisms revealed by their star formation histories
• Motion of small objects in curved spacetimes: An introduction to gravitational self-force
• Foreground cleaning and template-free stochastic background extraction for LISA
• Modelling neutron star mountains
• Hairy binary black holes in Einstein-Maxwell-dilaton theory and their effective-one-body description
• Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties
• Horizon-absorption effects in coalescing black-hole binaries: An effective-one-body study of the non-spinning case
• Post-Newtonian parameters gamma and beta of scalar-tensor gravity with a general potential
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Quasi-universal behaviour of the threshold mass in unequal-mass, spinning binary neutron-star mergers
• Incompleteness Matters Not: Inference of $H_0$ from BBH-galaxy cross-correlations
• Impact of Dynamical Tides on the Reconstruction of the Neutron Star Equation of State
• Three Dimensional Core-Collapse Supernova Simulations with 160 Isotopic Species Evolved to Shock Breakout
• Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise
• Black-hole kicks from numerical-relativity surrogate models
• Radiation reaction for spinning bodies in effective field theory I: Spin-orbit effects
• Probing planetary-mass primordial black holes with continuous gravitational waves
• Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current-neutrino interactions and inverse neutron decay
• Deep learning for multimessenger core-collapse supernova detection
• Rotating stellar core-collapse waveform decompositon: a Principal Component Analysis approach
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• A tale of two populations: Rotating Radio Transients and X-ray Dim Isolated Neutron Stars
• Characterising Transient Noise in the LIGO Detectors
• Merger of two neutron stars: predictions from the two-families scenario
• Emergence of microphysical bulk viscosity in binary neutron star post-merger dynamics
• Asteroseismology: radial oscillations of neutron stars with realistic equation of state
• Gravitational-wave surrogate models powered by artificial neural networks: The ANN-Sur for waveform generation
• Gamow-Teller strength in deformed nuclei within the self-consistent charge-exchange quasi-particle random-phase approximation with the Gogny force
• Nature of fault planes in solid neutron star matter
• Parameter Estimation and Model Selection of Gravitational Wave Signals Contaminated by Transient Detector Noise Glitches
• Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries
• Search for continuous gravitational waves from 20 accreting millisecond X-ray pulsars in O3 LIGO data
• Protostellar Feedback and Final Mass of the Second-Generation Primordial Stars
• Modeling ringdown II: non-precessing binary black holes
• Insights on Skyrme parameters from GW170817
• The enigmatic spin evolution of PSR J0537-6910: r-modes, gravitational waves and the case for continued timing
• Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos
• Resonantly enhanced and diminished strong-field gravitational-wave fluxes
• Tidal deformability and other global parameters of compact stars with strong phase transitions
• The clustering dynamics of primordial black boles in $N$-body simulations
• StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers
• Detection and Parameter Estimation of Gravitational Waves from Binary Neutron-Star Mergers in Real LIGO Data using Deep Learning
• Evolution of ONeMg Core in Super-AGB Stars towards Electron-Capture Supernovae: Effects of Updated Electron-Capture Rate
• A hybrid simulation of gravitational wave production in first-order phase transitions
• Towards inference of overlapping gravitational wave signals
• How common are long Gamma-Ray Bursts in the Local Universe?
• Black Holes Lessons from Multipole Ratios
• Gamma-ray burst jet propagation, development of angular structure, and the luminosity function
• CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• Quasiequilibrium sequences of binary neutron stars undergoing dynamical scalarization
• Exciting black hole modes via misaligned coalescences: I. Inspiral, transition, and plunge trajectories using a generalized Ori-Thorne procedure
• Strong gravitational lensing of gravitational waves in Einstein Telescope
• Machine Learning Gravitational Waves from Binary Black Hole Mergers
• g-mode Oscillations in Hybrid Stars: A Tale of Two Sounds
• Spanning the full range of neutron star properties within a microscopic description
• Gravitational Wave Bursts as Harbingers of Cosmic Strings Diluted by Inflation
• The Effect of Supernova Convection On Neutron Star and Black Hole Masses
• The presupernova core mass-radius relation of massive stars: understanding its formation and evolution
• Constraining First Star Formation with 21cm-Cosmology
• From Boundary Data to Bound States III: Radiative Effects
• Chirp Mass and Spin of Binary Black Holes from First Star Remnants
• Neutrino Flavor Evolution in Binary Neutron Star Merger Remnants
• Gravitational wave energy spectrum of hyperbolic encounters
• The Memory Remains (Undetected): Updates from the Second LIGO/Virgo Gravitational-Wave Transient Catalog
• Gravitational-wave sources from mergers of binary black-holes catalyzed by fly-bys interactions in the field
• Modelling frequency-dependent tidal deformability for environmental black-hole mergers
• Spin-induced dynamical scalarization, de-scalarization and stealthness in scalar-Gauss-Bonnet gravity during black hole coalescence
• Effectual gravitational-wave template banks for coalescing compact binaries using a hybrid placement algorithm
• How to assess the primordial origin of single gravitational-wave events with mass, spin, eccentricity, and deformability measurements
• Massively Parallel Simulations of Binary Black Hole Intermediate-Mass-Ratio Inspirals
• Black holes in the low mass gap: Implications for gravitational wave observations
• Cosmic String Loop Collapse in Full General Relativity
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• Uncertainty limits on neutron star radius measurements with gravitational waves
• Second-order gravitational self-force
• Gravitational-wave tail effects to quartic non-linear order
• Aligned spin neutron star-black hole mergers: a gravitational waveform amplitude model
• New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
• Circularization vs. Eccentrification in Intermediate Mass Ratio Inspirals inside Dark Matter Spikes
• Threshold of Primordial Black Hole Formation in Nonspherical Collapse
• Hyperbolicity of scalar-tensor theories of gravity
• Formation of black holes in the pair-instability mass gap: evolution of a post-collision star
• Primordial black hole formation during the QCD phase transition: threshold, mass distribution and abundance
• Stellar Mass Black Hole Formation and Multi-messenger Signals from Three Dimensional Rotating Core-Collapse Supernova Simulations
• A brief overview of black hole-neutron star mergers
• Gravitational Waves from Pati-Salam Dynamics
• Combined search for anisotropic birefringence in the gravitational-wave transient catalog GWTC-1
• Spherical harmonic modes of 5.5 post-Newtonian gravitational wave polarizations and associated factorized resummed waveforms for a particle in circular orbit around a Schwarzschild black hol
• The signal of the stochastic gravitational wave background and the angular correlation of its energy density
• Burial of the polar magnetic field of an accreting neutron star. II. Hydromagnetic stability of axisymmetric equilibria
• Anisotropies of gravitational-wave standard sirens as a new cosmological probe without redshift information
• The $N_{\ell }$ of gravitational wave background experiments
• Multi-messenger and multi-physics Bayesian inference for GW170817 binary neutron star merger
• What neutron stars tell about the hadron-quark phase transition: a Bayesian study
• Bayesian statistical framework for identifying strongly lensed gravitational-wave signals
• Second release of the CoRe database of binary neutron star merger waveforms
• Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations
• Exploring SMBH Assembly with Semi-analytic Modelling
• Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM
• Characteristic Time Variability of Gravitational-Wave and Neutrino Signals from Three-dimensional Simulations of Non-Rotating and Rapidly Rotating Stellar Core-Collapse
• Transmuted Gravity Wave Signals from Primordial Black Holes
• The progenitors of calcium-rich transients are not formed in situ
• Radiated momentum and radiation-reaction in gravitational two-body scattering including time-asymmetric effects
• Nonlinear/non-iterative treatment of EFT-motivated gravity
• Can LIGO Detect Non-Annihilating Dark Matter?
• Gravitational Radiations from a Spinning Compact Object around a supermassive Kerr black hole in circular orbit
• Frequency-domain algorithm for the Lorenz-gauge gravitational self-force
• Well-posedness of the four-derivative scalar-tensor theory of gravity in singularity avoiding coordinates
• Systematic uncertainty of standard sirens from the viewing angle of binary neutron star inspirals
• Possible Causes of False General Relativity Violations in Gravitational Wave Observations
• Shot noise in the astrophysical gravitational-wave background
• Searching for ultralight bosons within spin measurements of a population of binary black hole mergers
• Binary Neutron Stars with Arbitrary Spins in Numerical Relativity
• The quest for blue supergiants: binary merger models for the evolution of the progenitor of SN 1987A
• Conditions for Sustained Orbital Resonances in Extreme Mass Ratio Inspirals
• Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations
• Gravitational waves from hyperbolic encounters
• An instability due to the nonlinear coupling of p-modes to g-modes: Implications for coalescing neutron star binaries
• Multiband Observation of LIGO/Virgo Binary Black Hole Mergers in the Gravitational-wave Transient Catalog GWTC-1
• Waveform accuracy and systematic uncertainties in current gravitational wave observations
• Impact of high-order tidal terms on binary neutron-star waveforms
• Gravitational wave bursts from Primordial Black Hole hyperbolic encounters
• Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
• Mis-Modelling in Gravitational Wave Astronomy: The Trouble With Templates
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Gravitational waves from transient neutron star f-mode oscillations
• Tidal effects in the equations of motion of compact binary systems to next-to-next-to-leading post-Newtonian order
• Generalized framework for testing gravity with gravitational-wave propagation. III. Future prospect
• Applying the effective-source approach to frequency-domain self-force calculations: Lorenz-gauge gravitational perturbations
• Constraints on the distance duality relation with standard sirens
• Subtraction of correlated noise in global networks of gravitational-wave interferometers
• Asymptotic gravitational wave fluxes from a spinning particle in circular equatorial orbits around a rotating black hole
• Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
• In-depth analysis of the clustering of dark matter particles around primordial black holes I: density profiles
• Schwinger Effect by an $SU(2)$ Gauge Field during Inflation
• Gravitational wave signatures of dark matter cores in binary neutron star mergers by using numerical simulations
• Evolutionary Models for 43 Galactic Supernova Remnants with Distances and X-ray Spectra
• Dependence of outer boundary condition on protoneutron star asteroseismology with gravitational-wave signatures
• Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors
• Radio observations of extreme ULXs: revealing the most powerful ULX radio nebula ever or the jet of an intermediate-mass black hole?
• Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State
• Gaussian processes reconstruction of modified gravitational wave propagation
• Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code
• The Astrophysics of Resonant Orbits in the Kerr Metric
• Quantum gravity and gravitational-wave astronomy
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• Precessional instability in binary black holes with aligned spins
• Gravitational waves from global cosmic strings in quintessential inflation
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Merger of compact stars in the two-families scenario
• SuperRad: Modeling the black hole superradiance gravitational waveform
• The harmonic structure of generic Kerr orbits
• Kilonova Emission From Black Hole-Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches
• Targeted large mass ratio numerical relativity surrogate waveform model for GW190814
• Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae
• Status and perspectives of Continuous Gravitational Wave searches
• Dark Holograms and Gravitational Waves
• Exploring the small mass ratio binary black hole merger via Zeno's dichotomy approach
• Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
• Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks
• Results from the first all-sky search for continuous gravitational waves from small-ellipticity sources
• Order in the chaos: eccentric black hole binary mergers in triples formed via strong binary-binary scatterings
• The multipolar structure of fuzzballs
• Microscopic equation of state of hot nuclear matter for numerical relativity simulations
• Second-order perturbation theory: problems on large scales
• A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light boson clouds around spinning black holes
• Quantum Nuclear Pasta and Nuclear Symmetry Energy
• Modeling horizon absorption in spinning binary black holes using effective worldline theory
• Mode-by-mode Relative Binning: Fast Likelihood Estimation for Gravitational Waveforms with Spin-Orbit Precession and Multiple Harmonics
• Mapping dynamical ejecta and disk masses from numerical relativity simulations of neutron star mergers
• Non-Gaussianity from Axion-Gauge Fields Interactions during Inflation
• Towards numerical relativity in scalar Gauss-Bonnet gravity: 3+1 decomposition beyond the small-coupling limit
• The g-mode spectrum of reactive neutron star cores
• A "no-hair" test for binary black holes
• Gravitational waves from first-order phase transitions: Ultra-supercooled transitions and the fate of relativistic shocks
• Probing the incompressibility of nuclear matter at ultra-high density through the prompt collapse of asymmetric neutron star binaries
• Cosmological perturbation effects on gravitational-wave luminosity distance estimates
• Fast Frequency-domain Waveforms for Spin-Precessing Binary Inspirals
• Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
• Black Hole Formation in Fallback Supernova and the Spins of LIGO Sources
• Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
• Towards the nonlinear regime in extensions to GR: assessing possible options
• Non-parametric inference of the population of compact binaries from gravitational wave observations using binned Gaussian processes
• Higgsless simulations of cosmological phase transitions and gravitational waves
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model
• Primordial Black Hole Archaeology with Gravitational Waves from Cosmic Strings
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• Instability of Magnetic Equilibria in Barotropic Stars
• The Formation of Very Massive Stars in Early Galaxies and Implications for Intermediate Mass Black Holes
• Constraining the relativistic mean-field model equations of state with gravitational wave observations
• Tidal Deformability of Fermion-Boson Stars: Neutron Stars Admixed with Ultra-Light Dark Matter
• Improving gravitational-wave parameter estimation using Gaussian process regression
• The current-type quadrupole moment and gravitational-wave mode $(\ell ,m)=(2,1)$ of compact binary systems at the third post-Newtonian order
• Black hole merger simulations in wave dark matter environments
• Breaching the limit: formation of GW190521-like and IMBH mergers in young massive clusters
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Modeling dynamical scalarization with a resummed post-Newtonian expansion
• Magnification and evolution biases in large-scale structure surveys
• Reducing spurious gravitational radiation in binary-black-hole simulations by using conformally curved initial data
• Equations of state for hot neutron stars -- II. The role of exotic particle degrees of freedom
• Cosmic string loop shapes
• Gravitomagnetic tidal resonance in neutron-star binary inspirals
• The effects of host galaxy properties on merging compact binaries detectable by LIGO
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Tail contributions and post-adiabatic corrections
• Fuzzballs and Observations
• Modeling maximum astrophysical gravitational recoil velocities
• Hubble-induced phase transitions on the lattice with applications to Ricci reheating
• Black-hole remnants from black-hole--neutron-star mergers
• Search for nonlinear memory from subsolar mass compact binary mergers
• Extreme mass ratio inspirals on the equatorial plane in the adiabatic order
• Spin-spin effects in radiating compact binaries
• Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
• Eliminating the LIGO bounds on primordial black hole dark matter
• Irreducible background of gravitational waves from a cosmic defect network: update and comparison of numerical techniques
• A New Gravitational Wave Signature of Low-$T/|W|$ Instability in Rapidly Rotating Stellar Core Collapse
• Kicks and Induced Spins of Neutron Stars at Birth
• In-situ extreme mass ratio inspirals via sub-parsec formation and migration of stars in thin, gravitationally unstable AGN discs
• The Neutrino Response of Low-Density Neutron Matter from the Virial Expansion
• GRAthena++: puncture evolutions on vertex-centered oct-tree AMR
• Formation of LISA Black Hole Binaries in Merging Dwarf Galaxies: the Imprint of Dark Matter
• The SLUGGS Survey: Measuring globular cluster ages using both photometry and spectroscopy
• Thermal Effects in Binary Neutron Star Mergers
• A unified view of anisotropies in the astrophysical gravitational wave background
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• Merging stellar and intermediate-mass black holes in dense clusters: implications for LIGO, LISA and the next generation of gravitational wave detectors
• Inspiral into Gargantua
• Dissipation in extreme-mass ratio binaries with a spinning secondary
• Numerical simulation of sky localization for LISA-TAIJI joint observation
• Numerical simulations of the decay of primordial magnetic turbulence
• Gravitational-wave astronomy with a physical calibration model
• Universal relation for supernova gravitational waves
• Bayesian inference for gravitational waves from binary neutron star mergers in third-generation observatories
• Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case
• Measuring dark matter spikes around primordial black holes with Einstein Telescope and Cosmic Explorer
• Hidden Markov model tracking of continuous gravitational waves from young supernova remnants
• Lyman Alpha Signatures from Direct Collapse Black Holes
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• Strangeness-changing Rates and Hyperonic Bulk Viscosity in Neutron Star Mergers
• Jet Launching from Binary Neutron Star Mergers: Incorporating Neutrino Transport and Magnetic Fields
• On GLM curl cleaning for a first order reduction of the CCZ4 formulation of the Einstein field equations
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions
• Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity
• Neutrino emission from binary neutron star mergers: characterizing light curves and mean energies
• Numerical simulations of stellar collapse in scalar-tensor theories of gravity
• Discontinuous Galerkin method for computing gravitational waveforms from extreme mass ratio binaries
• Neutrinos and nucleosynthesis of elements
• Binary Pulsar constraints on massless scalar-tensor theories using Bayesian statistics
• Ready-to-use Fourier domain templates for compact binaries inspiraling along moderately eccentric orbits
• Motion in classical field theories and the foundations of the self-force problem
• A Precessing Numerical Relativity Waveform Surrogate Model for Binary Black Holes: A Gaussian Process Regression Approach
• On The Red Supergiant Problem
• Nearly extremal apparent horizons in simulations of merging black holes
• Stochastic constant-roll inflation and primordial black holes
• Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer
• A New Statistical Model for Population III Supernova Rates: Discriminating Between $\Lambda$CDM and WDM Cosmologies
• Generalized quasi-Keplerian solution for eccentric, non-spinning compact binaries at 4PN order and the associated IMR waveform
• Emerging chromo-natural inflation
• Nonlinear curvature effects in gravitational waves from inspiralling black hole binaries
• The spontaneous breaking of a metastable string
• On the motion of hairy black holes in Einstein-Maxwell-dilaton theories
• Domain walls seeding the electroweak phase transition
• Tidal response from scattering and the role of analytic continuation
• The First Billion Years of a Warm Dark Matter Universe
• Multi-band gravitational wave tests of general relativity
• Quasi-normal mode frequencies and gravitational perturbations of black holes with any subextremal spin in modified gravity through METRICS: the scalar-Gauss-Bonnet gravity case
• Multimessenger Cosmology: correlating CMB and SGWB measurements
• Comparison of post-Minkowskian and self-force expansions: Scattering in a scalar charge toy model
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Measuring precession in asymmetric compact binaries
• The final fate of stars that ignite neon and oxygen off-center: electron capture or iron core-collapse supernova?
• Self-Force in the Radiation Reaction Formula -- Adiabatic Approximation of a Metric Perturbation and an Orbit --
• Constraining self-interacting fermionic dark matter in admixed neutron stars using multimessenger astronomy
• Calculation of radiation reaction effect on orbital parameters in Kerr spacetime
• The stability of tidally deformed neutron stars to three- and four-mode coupling
• Cross-correlating Astrophysical and Cosmological Gravitational Wave Backgrounds with the Cosmic Microwave Background
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• Numerical relativity surrogate model with memory effects and post-Newtonian hybridization
• Do unequal-mass binary black hole systems have larger ${\chi }_{\text{eff}}$? Probing correlations with copulas in gravitational-wave astronomy
• Fragmentation induced starvation in Population III star formation: a resolution study
• Self-Force and Green Function in Schwarzschild spacetime via Quasinormal Modes and Branch Cut
• Real-time gravitational-wave inference for binary neutron stars using machine learning
• Spinning test body orbiting around a Kerr black hole: Eccentric equatorial orbits and their asymptotic gravitational-wave fluxes
• Multipole moments in scalar-tensor theory of gravity
• Two-step greedy algorithm for reduced order quadratures
• Inferring eccentricity evolution from observations of coalescing binary black holes
• The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
• Cosmological Effects of Radion Oscillations
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• A census of transient orbital resonances encountered during binary inspiral
• Logarithmic tail contributions to the energy function of circular compact binaries
• Sustained super-Eddington accretion in high-redshift quasars
• Constraining extra gravitational wave polarizations with Advanced LIGO, Advanced Virgo and KAGRA and upper bounds from GW170817
• Trapping of HII regions in Population III star formation
• Nonperturbative quark matter equations of state with vector interactions
• Application of hidden Markov model tracking to the search for long-duration transient gravitational waves from the remnant of the binary neutron star merger GW170817
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• Tests of gravitational symmetries with radio pulsars
• Maximum redshift of gravitational wave merger events
• Solving 3D relativistic hydrodynamical problems with WENO discontinuous Galerkin methods
• The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution
• Constraints on the maximum densities of neutron stars from postmerger gravitational waves with third-generation observations
• A double-domain spectral method for black hole excision data
• On the r-mode spectrum of relativistic stars
• Search for Continuous Gravitational Waves from Scorpius X-1 in LIGO O2 Data
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Gravitational waves from the collapse and bounce of a stellar core in tensor-scalar gravity
• Top-heavy integrated galactic stellar initial mass functions (IGIMFs) in starbursts
• Impact of gas hardening on the population properties of hierarchical black hole mergers in AGN disks
• Presupernova neutrinos: directional sensitivity and prospects for progenitor identification
• Superluminous supernovae: an explosive decade
• The Birthrate of Magnetars
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Searching for Standard Clocks in the Primordial Universe
• A Bayesian inference of relativistic mean-field model for neutron star matter from observation of NICER and GW170817/AT2017gfo
• Gravitational shine of dark domain walls
• Mass models of NGC 6624 without an intermediate-mass black hole
• Importance nested sampling with normalising flows
• Tidal deformability of boson stars and dark matter clumps
• Gravity in the infrared and effective nonlocal models
• Fast and Fourier: Extreme Mass Ratio Inspiral Waveforms in the Frequency Domain
• Gravitational Imprints of Flavor Hierarchies
• The sustainable growth of the first black holes
• Discovering gravitationally lensed gravitational waves: predicted rates, candidate selection, and localization with the Vera Rubin Observatory
• Second-order perturbation theory: the problem of infinite mode coupling
• Search for a scalar induced stochastic gravitational wave background in the third LIGO-Virgo observing run
• Accumulating errors in tests of general relativity with gravitational waves: overlapping signals and inaccurate waveforms
• A method to search for long duration gravitational wave transients from isolated neutron stars using the generalized FrequencyHough
• The Pre-Explosion Mass Distribution of Hydrogen-Poor Superluminous Supernova Progenitors and New Evidence for a Mass-Spin Correlation
• Standard-siren cosmology using gravitational waves from binary black holes
• The effect of wave dark matter on equal mass black hole mergers
• On how leakage can affect the Star Formation Rate estimation using Halpha luminosity
• On the four-loop static contribution to the gravitational interaction potential of two point masses
• The Ultimately Large Telescope -- what kind of facility do we need to detect Population III stars?
• Time-reversed particle-vibration loops and nuclear Gamow-Teller response
• Dynamical tides in coalescing superfluid neutron star binaries with hyperon cores and their detectability with third generation gravitational-wave detectors
• Dipolar tidal effects in scalar-tensor theories
• Comprehensive study of compact stars with dark matter
• Detection of a $\sim$100,000 M${}_{\odot }$ black hole in M31's most massive globular cluster: A tidally stripped nucleus
• The cluster structure of the inner crust of neutron stars in the Hartree-Fock-Bogoliubov approach
• Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
• Novel Method for Incorporating Model Uncertainties into Gravitational Wave Parameter Estimates
• IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient Catalog
• Polarization of a stochastic gravitational wave background through diffusion by massive structures
• Improvements to the construction of binary black hole initial data
• ALMA spectral survey of Supernova 1987A --- molecular inventory, chemistry, dynamics and explosive nucleosynthesis
• Crystallization of the inner crust of a neutron star and the influence of shell effects
• Global cosmic string networks as a function of tension
• A Potential Progenitor for the Type Ic Supernova 2017ein
• Observations of SN 2017ein Reveal Shock Breakout Emission and A Massive Progenitor Star for a Type Ic Supernova
• Tests of general relativity using multiband observations of intermediate mass binary black hole mergers
• Oscillatory features in the curvature power spectrum after a sudden turn of the inflationary trajectory
• Self-consistent 3D radiative transfer for kilonovae: directional spectra from merger simulations
• The mass quadrupole moment of compact binary systems at the fourth post-Newtonian order
• Modelling neutron star mountains in relativity
• Deep Einstein@Home all-sky search for continuous gravitational waves in LIGO O3 public data
• Formation and merging of Mass Gap Black Holes in Gravitational Wave Merger Events from Wide Hierarchical Quadruple Systems
• Dynamical ejecta synchrotron emission as possible contributor to the changing behaviour of GRB170817A
• Exploring the Properties of Choked Gamma-Ray Bursts with IceCube's High Energy Neutrinos
• Investigating the retention of intermediate-mass black holes in star clusters using N-body simulations
• Spin effects in the phasing of gravitational waves from binaries on eccentric orbits
• Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh: II. Time-reversal symmetry breaking
• Improved next-to-leading order tidal heating and torquing of a Kerr black hole
• VAMANA: Modeling Binary Black Hole Population with Minimal Assumptions
• Fission and the r-process nucleosynthesis of translead nuclei in neutron star mergers
• Noisy neighbours: inference biases from overlapping gravitational-wave signals
• Discovery of a 760 nm P Cygni line in AT2017gfo: Identification of yttrium in the kilonova photosphere
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• Constructing Binary Neutron Star Initial Data with High Spins, High Compactness, and High Mass-Ratios
• Termination of Superradiance from a Binary Companion
• Accretion-induced spin-wandering effects on the neutron star in Scorpius X-1: Implications for continuous gravitational wave searches
• Quadrupole moment of a magnetically confined mountain on an accreting neutron star: effect of the equation of state
• Gravitational radiation from compact binary systems in Einstein-Maxwell-dilaton theories
• Catastrogenesis: DM, GWs, and PBHs from ALP string-wall networks
• Optimization of seismometer arrays for the cancellation of Newtonian noise from seismic body waves
• Modelling self-consistently beyond General Relativity
• Strong-field scattering of two spinning black holes: Numerics versus Analytics
• Observational Inference on the Delay Time Distribution of Short Gamma-ray Bursts
• Searching for Fossil Fields in the Gravity Sector
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Detecting the QCD phase transition in the next Galactic supernova neutrino burst
• Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering
• Searching for mass-spin correlations in the population of gravitational-wave events: the GWTC-3 case study
• Adiabatic Evolution of three 'Constants' of Motion for Greatly Inclined Orbits in Kerr spacetime
• Scaling properties of cosmological axion strings
• Cosmic Strings
• Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties
• Double Compact Objects as Low-frequency Gravitational Wave Sources
• Impact of the Primordial Stellar Initial Mass Function on the 21-cm Signal
• Probing ultralight dark matter with future ground-based gravitational-wave detectors
• Second-order gravitational self-force in a highly regular gauge
• physiCal: A physical approach to the marginalization of LIGO calibration uncertainties
• Spectral analysis of gravitational waves from binary neutron star merger remnants
• Binary black hole spectroscopy: a no-hair test of GW190814 and GW190412
• Subtraction-noise projection in gravitational-wave detector networks
• Resistive relaxation of a magnetically confined mountain on an accreting neutron star
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Tensor non-Gaussianity in chiral scalar-tensor theories of gravity
• Quantum rotating black holes
• The swallowing of a quark star by a black hole
• Ringing out General Relativity: Quasi-normal mode frequencies for black holes of any spin in modified gravity
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Validity of common modelling approximations for precessing binary black holes with higher-order modes
• Spin effects in gravitational waveforms and fluxes for binaries on eccentric orbits to the third post-Newtonian order
• Primordial production of massive relic gravitational waves from a weak modification of General Relativity
• Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project
• EoS for hot neutron stars
• Dynamical Formation of Scalarized Black Holes and Neutron Stars through Stellar Core Collapse
• Multi-flavour SMBH seeding and evolution in cosmological environments
• Fast time variations of supernova neutrino signals from 3-dimensional models
• Quasiequilibrium sequences of black-hole--neutron-star binaries in general relativity
• Nucleonic metamodelling in light of multimessenger, PREX-II and CREX data
• The star clusters that make black hole binaries across cosmic time
• The state of matter in simulations of core-collapse supernovae -- Reflections and recent developments
• Impact of the wave-like nature of Proca stars on their gravitational-wave emission
• On accretion disks formed in MHD simulations of black hole-neutron star mergers with accurate microphysics
• Central kinematics of the globular cluster NGC 2808: Upper limit on the mass of an intermediate-mass black hole
• Formation of supermassive stars in the first star clusters
• Multiband gravitational-wave searches for ultralight bosons
• Gravitational Wave "Echo" Spectra
• Unveiling early black hole growth with multi-frequency gravitational wave observations
• $\Delta$-admixed neutron stars: spinodal instabilities and dUrca processes
• Influence of the crust on the neutron star macrophysical quantities and universal relations
• The stochastic gravitational wave background from close hyperbolic encounters of primordial black holes in dense clusters
• Gravitational waves from rotating neutron stars
• Crystallization of the outer crust of a non-accreting neutron star
• Rapid Black Hole Spin-down by Thick Magnetically Arrested Disks
• Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3
• Flexible and Fast Estimation of Binary Merger Population Distributions with Adaptive KDE
• GRMHD large eddy simulations with gradient subgrid-scale model
• Effective spin distribution of black hole mergers in triples
• Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
• Interaction of misaligned magnetospheres in the coalescence of binary neutron stars
• A new code for equilibriums and quasiequilibrium initial data of compact objects
• An efficient iterative method to reduce eccentricity in numerical-relativity simulations of compact binary inspiral
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
• On the single-event-based identification of primordial black hole mergers at cosmological distances
• Lorenz gauge gravitational self-force calculations of eccentric binaries using a frequency domain procedure
• (Sort of) Testing relativity with extreme mass ratio inspirals
• Orbital resonances around Black holes
• Frequency response of space-based interferometric gravitational-wave detectors
• Two-body problem in Scalar-Tensor theories as a deformation of General Relativity : an Effective-One-Body approach
• Analytic gravitational waveforms for generic precessing compact binaries
• Comparing Effective One Body Hamiltonians for spin-aligned coalescing binaries
• Factorization and resummation: A new paradigm to improve gravitational wave amplitudes. II: the higher multipolar modes
• Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins
• Accelerating the evaluation of inspiral-merger-ringdown waveforms with adapted grids
• P not PQ
• Gauge invariant formulation of gravitational waves in metric $f(R)$ gravity
• Normalizing flows as an avenue to study overlapping gravitational wave signals
• Improved sensitivity of interferometric gravitational wave detectors to ultralight vector dark matter from the finite light-traveling time
• Double neutron star mergers from hierarchical triple-star systems
• Tests of general relativity with stellar-mass black hole binaries observed by LISA
• Ultralight bosons for strong gravity applications from simple Standard Model extensions
• On the radio properties of the intermediate-mass black hole candidate ESO 243-49 HLX-1
• Beyond freeze-in: Dark Matter via inverse phase transition and gravitational wave signal
• Starbursts in low-mass haloes at Cosmic Dawn. I. The critical halo mass for star formation
• Gravitational waves from spinning compact binaries in hyperbolic orbits
• What You Don't Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses
• Pre-merger localization of compact-binary mergers with third generation observatories
• Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
• Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube
• Measuring the delay time distribution of binary neutron stars. II. Using the redshift distribution from third-generation gravitational wave detectors network
• Black Hole Binaries in Cubic Horndeski Theories
• Quasinormal modes of compact objects in alternative theories of gravity
• Exploring the sky localization and early warning capabilities of third generation gravitational wave detectors in three-detector network configurations
• Gravitational-wave detectors as particle-physics laboratories: Constraining scalar interactions with a coherent inspiral model of boson-star binaries
• Dynamic Normalization for Compact Binary Coalescence Searches in Non-Stationary Noise
• Generalized Uncertainty Principle and White Dwarfs Redux: How Cosmological Constant Protects Chandrasekhar Limit
• Coherent neutrino radiation in supernovae at two loops
• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
• Analytic models of the spectral properties of gravitational waves from neutron star merger remnants
• Quantisation Across Bubble Walls and Friction
• Compact Dark Objects in Neutron Star Mergers
• Cross-correlating galaxy catalogs and gravitational waves: a tomographic approach
• Search for black hole hyperbolic encounters with gravitational wave detectors
• Cosmological inference from standard sirens without redshift measurements
• Gravitational Wave mergers as tracers of Large Scale Structures
• How to search for gravitational waves from $r$-modes of known pulsars
• Assessing the Readiness of Numerical Relativity for LISA and 3G Detectors
• Dimension dependence of numerical simulations on gravitational waves from protoneutron stars
• Avoided crossing in gravitational wave spectra from protoneutron star
• Impact of Numerical Relativity information on effective-one-body waveform models
• Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3b
• Bulk viscosity from Urca processes: $npe\mu$ matter in the neutrino-trapped regime
• The role of jets in exploding supernovae and in shaping their remnants
• Reducing the two-body problem in scalar-tensor theories to the motion of a test particle : a scalar-tensor effective-one-body approach
• "Flux-balance formulae" for extreme mass-ratio inspirals
• Testing the Early Universe with Anisotropies of the Gravitational Wave Background
• Motion and gravitational wave forms of eccentric compact binaries with orbital-angular-momentum-aligned spins under next-to-leading order in spin-orbit and leading order in spin(1)-spin(2) and spin-squared couplings
• Gravitational wave signatures from discrete flavor symmetries
• Testing general relativity with gravitational-wave catalogs: the insidious nature of waveform systematics
• Dynamical evolution of Population III stellar systems and the resulting binary statistics
• NGC 4993, the shell galaxy host of GW170817: constraints on the recent galactic merger
• Primordial features and Planck polarization
• Denoising Gravitational Waves using Deep Learning with Recurrent Denoising Autoencoders
• Denoising Gravitational Waves with Enhanced Deep Recurrent Denoising Auto-Encoders
• Untangling features in the primordial spectra
• Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
• Recognizing black holes in gravitational-wave observations: Challenges in telling apart impostors in mass-gap binaries
• General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
• Exploring the hidden Universe: A novel phenomenological approach for recovering arbitrary gravitational-wave millilensing configurations
• Cusp-to-core transition in low-mass dwarf galaxies induced by dynamical heating of cold dark matter by primordial black holes
• Ultrahigh frequency primordial gravitational waves beyond the kHz: The case of cosmic strings
• Uncovering the History of Cosmic Inflation from Anomalies in Cosmic Microwave Background Spectra
• Tail contributions to gravitational conservative dynamics
• Search of the Early O3 LIGO Data for Continuous Gravitational Waves from the Cassiopeia A and Vela Jr. Supernova Remnants
• Second post-Newtonian order radiative dynamics of inspiralling compact binaries in the Effective Field Theory approach
• Third post-Newtonian effective-one-body Hamiltonian in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity
• Very fast stochastic gravitational wave background map making using folded data
• Gravitational waves from single neutron stars: an advanced detector era survey
• Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors
• Impacts of overlapping gravitational-wave signals on the parameter estimation: Toward the search for cosmological backgrounds
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• A Blast from the Pasture: Studying the environment of AT 2018cow with MUSE
• Primordial Black Holes as Silver Bullets for New Physics at the Weak Scale
• Constraining pre Big-Bang-Nucleosynthesis Expansion using Cosmic Antiprotons
• Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraints
• Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• Binary neutron star mergers in Einstein-scalar-Gauss-Bonnet gravity
• Computing Fast and Reliable Gravitational Waveforms of Binary Neutron Star Merger Remnants
• Transition from adiabatic inspiral to plunge into a spinning black hole
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• Formation of super-massive black holes in galactic nuclei I: delivering seed intermediate-mass black holes in massive stellar clusters
• Three-dimensional core-collapse supernovae with complex magnetic structures: II. Rotational instabilities and multi-messenger signatures
• "Super-Kilonovae" from Massive Collapsars as Signatures of Black-Hole Birth in the Pair-instability Mass Gap
• Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics
• Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission
• Completing the Fifth PN Precision Frontier via the EFT of Spinning Gravitating Objects
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Spin contributions to the gravitational-waveform modes for spin-aligned binaries at the 3.5PN order
• An effective action model of dynamically scalarizing binary neutron stars
• Impact of the neutron-star deformability on equation of state parameters
• Testing Gravitational Memory Generation with Compact Binary Mergers
• Spins of primordial black holes formed in different cosmological scenarios
• Integrated Sachs-Wolfe Effect for Gravitational Radiation
• The Kepler equation for inspiralling compact binaries
• On modeling for Kerr black holes: Basis learning, QNM frequencies, and spherical-spheroidal mixing coefficients
• Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
• Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
• Horizon-absorbed energy flux in circularized, nonspinning black-hole binaries and its effective-one-body representation
• Unveiling the merger structure of black hole binaries in generic planar orbits
• Gravitomagnetic tidal effects in gravitational waves from neutron star binaries
• Comparing Accretion Disks and Dark Matter Spikes in Intermediate Mass Ratio Inspirals
• Astrophysical science metrics for next-generation gravitational-wave detectors
• Assessing the model waveform accuracy of gravitational waves
• Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding
• Expansion history-dependent oscillations in the scalar-induced gravitational wave background
• Second Einstein Telescope Mock Data and Science Challenge: Low Frequency Binary Neutron Star Data Analysis
• Gravitational traces of broken gauge symmetries
• Direct determination of cosmic string loop density from simulations
• Fermion soliton stars
• Improved deep learning techniques in gravitational-wave data analysis
• Evidence for the evolution of black hole mass function with redshift
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
• Gravitational-wave flux for a particle orbiting a Kerr black hole to 20th post-Newtonian order: a numerical approach
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• Bayesian inference of signatures of hyperons inside neutron stars
• Self-force via Green functions and worldline integration
• Evolution of binary systems accompanying axion clouds in extreme mass ratio inspirals
• Ruling out Initially Clustered Primordial Black Holes as Dark Matter
• Impact of noise transients on low latency gravitational-wave event localisation
• The Eccentric Behavior of Inspiraling Compact Binaries
• The dynamo effect in decaying helical turbulence
• Sudden variations in the speed of sound during inflation: features in the power spectrum and bispectrum
• Developing a model for neutron star oscillations following starquakes
• Reply to "Comment on 'Universality of Quantum Gravity Corrections' "
• Implementing a semicoherent search for continuous gravitational waves using optimally-constructed template banks
• Signatures of ultralight bosons in the orbital eccentricity of binary black holes
• Improving the background of gravitational-wave searches for core collapse supernovae: A machine learning approach
• Dynamical descalarization with a jump during black hole merger
• Modeling Supermassive Primordial Stars with MESA
• The extended radio jet of an off-nuclear low-mass AGN in NGC 5252
• Radiation from Global Topological Strings using Adaptive Mesh Refinement: Methodology and Massless Modes
• Inferring fundamental spacetime symmetries with gravitational-wave memory: from LISA to the Einstein Telescope
• Spectral method for metric perturbations of black holes: Kerr background case in general relativity
• Bubble wall velocity during electroweak phase transition in the inert doublet model
• A synthetic model of the gravitational wave background from evolving binary compact objects
• Friction on ALP domain walls and gravitational waves
• Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy
• New effective precession spin for modeling multimodal gravitational waveforms in the strong-field regime
• Quantum Hair from Gravity
• Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy
• Characterisation of lensing selection effects for LISA massive black hole binary mergers
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• Fixing the dynamical evolution in scalar-Gauss-Bonnet gravity
• Gravitational wave friction in light of GW170817 and GW190521
• Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing binary black hole coalescence
• Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants
• Enhancing gravitational wave anisotropies with peaked scalar sources
• The observed mass distribution of Galactic black hole LMXBs is biased against massive black holes
• Prospects for determining the nature of the secondaries of extreme mass-ratio inspirals using the spin-induced quadrupole deformation
• Three-dimensional stability of magnetically confined mountains on accreting neutron stars
• The Case for Hypercritical Accretion in M33 X-7
• Neutron Star Crust Can Support A Large Ellipticity
• Self-force correction to the deflection angle in black-hole scattering: a scalar charge toy model
• The mass and angular momentum of reconstructed metric perturbations
• Sinking of a magnetically confined mountain on an accreting neutron star
• IceCube search for neutrinos coincident with gravitational wave events from LIGO/Virgo run O3
• The Formation of Rapidly Rotating Black Holes in High Mass X-ray Binaries
• Applying the effective-source approach to frequency-domain self-force calculations
• General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking
• Fast Gravitational Wave Radiometry using Data Folding
• All-sky search for long-duration gravitational-wave transients in the second Advanced LIGO observing run
• Simple procedures to reduce eccentricity of binary black hole simulations
• Probing gravitational wave polarizations with Advanced LIGO, Advanced Virgo and KAGRA
• Formulating bulk viscosity for neutron star simulations
• UV completions, fixing the equations and nonlinearities in $k$-essence
• Dynamical tides in neutron stars: The impact of the crust
• Gravitational radiation reaction in compact binary systems: Contribution of the quadrupole-monopole interaction
• Dependence of weak interaction rates on the nuclear composition during stellar core collapse
• Constraints on the ultralight scalar boson from Advanced LIGO and Advanced Virgo's first three observing runs using the stochastic gravitational-wave background
• Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars
• Urca reactions during neutron star inspiral
• Spectral Method for the Gravitational Perturbations of Black Holes: Schwarzschild Background Case
• Primordial black hole dark matter from catastrogenesis with unstable pseudo-Goldstone bosons
• Bounds on GUP parameters from GW150914 and GW190521
• The Adaptive Transient Hough method for long-duration gravitational wave transients
• Gravitational perturbations of rotating black holes in Lorenz gauge
• Modeling transient resonances in extreme-mass-ratio inspirals
• Resonant Signatures of Heavy Scalar Fields in the Cosmic Microwave Background
• Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and $\mathbf{\gamma }$-Ray Bursts
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
• Isolated and dynamical black hole mergers with \texttt{B-POP}: the role of star formation and dynamics, star cluster evolution, natal kicks, mass and spins, and hierarchical mergers
• Gravitational waveforms for spinning compact binaries
• Towards Rapid Parameter Estimation on Gravitational Waves from Compact Binaries using Interpolated Waveforms
• All-sky, all-frequency directional search for persistent gravitational-waves from Advanced LIGO's and Advanced Virgo's first three observing runs
• Phase transitions in perturbative walking dynamics
• Revisiting the evidence for precession in GW200129 with machine learning noise mitigation
• Relativistic effective action of dynamical gravitomagnetic tides for slowly rotating neutron stars
• Excitation of f-modes during mergers of spinning binary neutron star
• Holographic Bubbles with Jecco: Expanding, Collapsing and Critical
• Primordial spectra from sudden turning trajectory
• Probing Two-Field Open Inflation by Resonant Signals in Correlation Functions
• Probing internal dissipative processes of neutron stars with gravitational waves during the inspiral of neutron star binaries
• Neutron Star-Black Hole Mergers from Gravitational Wave Captures
• Cosmic Evolution of Stellar-mass Black Hole Merger Rate in Active Galactic Nuclei
• Gravitational-wave tails of memory
• Low-Scale Leptogenesis and the Domain Wall Problem in Models with Discrete Flavor Symmetries
• The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources
• Milliarcsec-scale radio emission of ultraluminous X-ray sources: steady jet emission from an intermediate-mass black hole?
• Gravitational wave propagation in $f(R)$ models: New parametrizations and observational constraints
• Insights into non-axisymmetric instabilities in three-dimensional rotating supernova models with neutrino and gravitational-wave signatures
• Cosmography using strongly lensed gravitational waves from binary black holes
• Landscape of stellar-mass black-hole spectroscopy with third-generation gravitational-wave detectors
• Bayesian Inference of the Dense Matter Equation of State built upon Covariant Density Functionals
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• The host galaxies of double compact objects across cosmic time
• A Simple method to set up low eccentricity initial data for moving puncture simulations
• R-axion detection at LHC
• General relativistic dynamical tides in binary inspirals, without modes
• Ultra long lived quasinormal modes of neutron stars in massive scalar-tensor gravity
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: From Source to Canonical Moment
• Effects of the standing accretion-shock instability and the lepton-emission self-sustained asymmetry in the neutrino emission of rotating supernovae
• Hereditary Effects in Eccentric Compact Binary Inspirals to Third Post-Newtonian Order
• Effect of clustering on primordial black hole microlensing constraints
• Disentangling the formation mechanisms of nuclear star clusters
• Unblocking of stellar electron capture for neutron-rich $N=50$ nuclei at finite temperature
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• New code for equilibriums and quasiequilibrium initial data of compact objects. IV. Rotating relativistic stars with mixed poloidal and toroidal magnetic fields
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• Nonspinning black hole-neutron star mergers: a model for the amplitude of gravitational waveforms
• A strong He II $\lambda$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?
• Constraining equation of state groups from $g$-mode asteroseismology
• Gravitational waves $\times$ HI intensity mapping: cosmological and astrophysical applications
• Primordial Standard Clock Models and CMB Residual Anomalies
• Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos
• Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models
• Robust statistics for deterministic and stochastic gravitational waves in non-Gaussian noise. II: Bayesian analyses
• Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
• Gauge and motion in perturbation theory
• On the Evolution of Supermassive Primordial Stars in Cosmological Flows
• Microlensing of gravitational waves by dark matter structures
• Large Eddy Simulations of Magnetized Mergers of Neutron Stars with Neutrinos
• Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
• Asymmetric accretion and thermal `mountains' in magnetized neutron star crusts
• Nonlocal gravity and gravitational-wave observations
• Dancing in the dark: detecting a population of distant primordial black holes
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: II. Dimensional Regularization and Renormalization
• Formation of Globular Cluster Systems II: Impact of the Cutoff of the Cluster Initial Mass Function
• Probing new light gauge bosons with gravitational-wave interferometers using an adapted semi-coherent method
• Gravitational backreaction simulations of simple cosmic string loops
• Circular polarizations of gravitational waves from core-collapse supernovae: a clear indication of rapid rotation
• Inferring the core-collapse supernova explosion mechanism with three-dimensional gravitational-wave simulations
• Impact of Schumann resonances on the Einstein Telescope and projections for the magnetic coupling function
• Phase conversion dissipation in multicomponent compact stars
• Supernova matter at subnuclear densities as a resonant Fermi gas: Enhancement of neutrino rates
• Inferring the neutron star maximum mass and lower mass gap in neutron star-black hole systems with spin
• Timing the Neutrino Signal of a Galactic Supernova
• Factorization and resummation: A new paradigm to improve gravitational wave amplitudes. III: the spinning test-body terms
• Cosmography with next-generation gravitational wave detectors
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• Intermediate-mass-ratio-inspirals in the Einstein Telescope. II. Parameter estimation errors
• An Optical Study of the Black Widow Population
• Post-Minkowskian Theory Meets the Spinning Effective-One-Body Approach for Two-Body Scattering
• Radio Observations of Supernova Remnant G1.9+0.3
• Computing waveforms for spinning compact binaries in quasi-eccentric orbits
• Boundary to bound dictionary for generic Kerr orbits
• Fundamental physics and the absence of sub-millisecond pulsars
• The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history
• High Quality QCD Axion at Gravitational Wave Observatories
• Testing gravitational wave propagation with multiband detections
• Multimessenger Asteroseismology of Core-Collapse Supernovae
• Explaining Nonlinearities in Black Hole Ringdowns from Symmetries
• Erratum: Progenitor-explosion connection and remnant birth masses for neutrino-driven supernovae of iron-core progenitors (2012, ApJ, 757, 69)
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
• Massive Black Hole Seeds
• A gravitational-wave limit on the Chandrasekhar mass of dark matter
• A statistical view on stable and unstable Roche lobe overflow of a tertiary star onto the inner binary in triple systems
• A Study of Primordial Very Massive Star Evolution
• An analytic family of post-merger template waveforms
• Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
• Clustering of primordial black holes from quantum diffusion during inflation
• Looking for the parents of LIGO's black holes
• Gravitational waves from color-magnetic `mountains' in neutron stars
• Complex dimensions and their observability
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• Continuous gravitational waves from Galactic neutron stars: demography, detectability and prospects
• First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
• Long-term 3D-MHD Simulations of Black Hole Accretion Disks formed in Neutron Star Mergers
• Common-envelope Dynamics of a Stellar-mass Black Hole: General Relativistic Simulations
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• Effective-one-body waveforms for extreme-mass-ratio binaries: Consistency with second-order gravitational self-force quasicircular results and extension to nonprecessing spins and eccentricity
• Mixed Non-Gaussianity from Axion-Gauge Field Dynamics
• Inspiralling eccentric binary neutron stars: orbital motion and tidal resonance
• Nearly model-independent constraints on dense matter equation of state in a Bayesian approach
• Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks
• The impact of the FMR and starburst galaxies on the (low-metallicity) cosmic star formation history
• Empirical constraints on the high-density equation of state from multi-messenger observables
• Constraints on high density equation of state from maximum neutron star mass
• Regression methods in waveform modeling: a comparative study
• Tossing Black Hole Spin Axes
• A new effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
• Gravitational radiation from neutron stars deformed by crustal Hall drift
• Compact Object Modeling in the Globular Cluster 47 Tucanae
• Identifying rotation in SASI-dominated core-collapse supernovae with a neutrino gyroscope
• A Linear and Quadratic Time-Frequency Analysis of Gravitational Waves from Core-Collapse Supernovae
• Formation, disruption and energy output of Population III X-ray binaries
• Optimization of model independent gravitational wave search using machine learning
• Binary Neutron Stars Gravitational Wave Detection Based on Wavelet Packet Analysis And Convolutional Neural Networks
• Leveraging gravitational-wave memory to distinguish neutron star--black hole binaries from black hole binaries
• Prospects for gravitational-wave polarization test from compact binary mergers with future ground-based detectors
• Comparing multi-field primordial feature models with the Planck data
• Formation of black holes in the pair-instability mass gap: Hydrodynamical simulations of a head-on massive star collision
• Core collapse in massive scalar-tensor gravity
• Comparison of binary black hole initial data sets
• Use and Abuse of the Model Waveform Accuracy Standards
• Dynamical Love for area quantized black holes
• Testing Primordial Black Holes with multi-band observations of the stochastic gravitational wave background
• Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations
• How loud are echoes from exotic compact objects?
• Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
• Hydrodynamic backreaction force of cosmological bubble expansion
• Temperature dependence of nuclear spin-isospin response and beta decay in hot astrophysical environments
• The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
• Demographics of neutron stars in young massive and open clusters
• Magnetar Asteroseismology with Long-Term Gravitational Waves
• Assessing the Energetics of Spinning Binary Black Hole Systems
• Hubble-induced phase transitions: Walls are not forever
• Impact of multiple modes on the evolution of self-interacting axion condensate around rotating black holes
• Circular polarization of gravitational waves from non-rotating supernova cores: a new probe into the pre-explosion hydrodynamics
• Transport properties of nuclear pasta phase with quantum molecular dynamics
• Binary neutron star mergers as a probe of quark-hadron crossover equations of state
• Transient gravitational waves from pulsar post-glitch recoveries
• Massive black hole assembly in nuclear star clusters
• Doppler boosting the stochastic gravitational wave background
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• Analytic solutions for the motion of spinning particles near spherically symmetric black holes and exotic compact objects
• Nambu-Goto Dynamics of Field Theory Cosmic String Loops
• Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
• Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope
• Primordial Black Holes from Thermal Inflation
• Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel
• nEoS: Neutron Star Equation of State from hadron physics alone
• Theoretical prediction of presupernova neutrinos and their detection
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Classifying the Equation of State from Rotating Core Collapse Gravitational Waves with Deep Learning
• Gravitational Waves from Core-Collapse Supernovae
• Black hole - black hole total merger mass and the origin of LIGO/Virgo sources
• Energy-conservation constraints on cosmic string loop production and distribution functions
• Aligned Spins: Orbital Elements, Decaying Orbits, and Last Stable Circular Orbit to high post-Newtonian Orders
• Model-Independent Inference of Neutron Star Radii from Moment of Inertia Measurements
• Detecting primordial features with LISA
• Bulk Viscosity of Relativistic $npe\mu$ Matter in Neutron-Star Mergers
• Relic gravitational waves from the chiral magnetic effect
• Gravitational wave populations and cosmology with neural posterior estimation
• Estimating the Neutrino Flux from Choked Gamma-Ray Bursts
• Quasinormal modes of Kerr black holes using a spectral decomposition of the metric perturbations
• Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamics Simulations
• LSTM and CNN application for core-collapse supernova search in gravitational wave real data
• Properties of the remnant disk and the dynamical ejecta produced in low-mass black hole-neutron star mergers
• Heavy primordial black holes from strongly clustered light black holes
• Entropy density of spacetime from the zero point length
• Signatures of primordial black holes in gravitational wave clustering
• Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
• Circular Polarization of the Astrophysical Gravitational Wave Background
• Stellar electron capture rates on neutron-rich nuclei and their impact on core-collapse
• Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors
• Resonant self-force effects in extreme-mass-ratio binaries: A scalar model
• Localized Features in Non-Gaussianity from Heavy Physics
• Massive binary black holes from Population II and III stars
• No velocity-kicks are required to explain large-distance offsets of Ca-rich supernovae and short-GRBs
• Constraining Nuclear Symmetry Energy with Multi-messenger Resonant Shattering Flares
• Gravitational wave hints black hole remnants as dark matter
• Gravitational Collider Physics via Pulsar-Black Hole Binaries
• A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity
• Probing Early Universe Supercooled Phase Transitions with Gravitational Wave Data
• First constraint on the dissipative tidal deformability of neutron stars
• Interpolating compact binary waveforms using the singular value decomposition
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Cross-correlations as a Diagnostic Tool for Primordial Gravitational Waves
• Theory-agnostic framework for dynamical scalarization of compact binaries
• Fundamental frequencies and resonances from eccentric and precessing binary black hole inspirals
• Practical approaches to analyzing PTA data: Cosmic strings with six pulsars
• Dynamics of F/D networks: the role of bound states
• Tidal effects up to next-to-next-to leading post-Newtonian order in massless scalar-tensor theories
• Microlensing constraints on clustered primordial black holes
• Investigating tidal heating in neutron stars via gravitational Raman scattering
• K-dynamics: well-posed 1+1 evolutions in K-essence
• Compact object binary mergers driven by cluster tides: a new channel for LIGO/Virgo gravitational wave events
• Finding Direct-Collapse Black Holes at Birth
• Impact of massive neutron star radii on the nature of phase transitions in dense matter
• Less than 1% of Core-Collapse Supernovae in the local universe occur in elliptical galaxies
• On the population III binary black hole mergers beyond the pair-instability mass gap
• Stochastic gravitational wave background constraints from Gaia DR3 astrometry
• Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• Testing the"no-hair" nature of binary black holes using the consistency of multipolar gravitational radiation
• Gravitational waves from mountains in newly born millisecond magnetars
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• New universal property of cosmological gravitational wave anisotropies
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM
• Ultra-compact X-ray binaries as dual-line gravitational-wave sources
• Reduced Order and Surrogate Models for Gravitational Waves
• Rapid neutron star cooling triggered by dark matter
• Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors
• Adiabatic equatorial inspirals of a spinning body into a Kerr black hole
• Impact of systematic nuclear uncertainties on composition and decay heat of dynamical and disk ejecta in compact binary mergers
• Model-based cross-correlation search for gravitational waves from the low-mass X-ray binary Scorpius X-1 in LIGO O3 data
• Gravitational Waves from Current-Carrying Cosmic Strings
• Impact of pions on binary neutron star mergers
• Quasi-extremal primordial black holes are a viable dark matter candidate
• Gravitational waves from spinning eccentric binaries
• Globular cluster formation histories, masses and radii inferred from gravitational waves
• Gravitational Wave Signals from Two-Dimensional Core-Collapse Supernova Models with Rotation and Magnetic Fields
• Improved neutrino-nucleon interactions in dense and hot matter for numerical simulations
• Stable mass transfer can explain massive binary black hole mergers with a high spin component
• An autoencoder neural network integrated into gravitational-wave burst searches to improve the rejection of noise transients
• Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
• Two-Moment Neutrino Flavor Transformation with applications to the Fast Flavor Instability in Neutron Star Mergers
• Gravitational waves from spinning binary black holes at the leading post-Newtonian orders at all orders in spin
• Precision Early Universe Cosmology from Stochastic Gravitational Waves
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• Pre-merger alert to detect the very-high-energy prompt emission from binary neutron-star mergers: Einstein Telescope and Cherenkov Telescope Array synergy
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: Relating the Harmonic and Radiative Metrics
• Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO
• Axial quasi-normal modes of scalarized neutron stars with massive self-interacting scalar field
• Modeling Core-Collapse Supernovae Gravitational-Wave Memory in Laser Interferometric Data
• Searching for gravitational wave bursts from cosmic string cusps with the Parkes Pulsar Timing Array
• Logarithmically divergent friction on ultrarelativistic bubble walls
• Gravitational Wave Emission from a Cosmic String Loop, I: Global Case
• Self-force framework for transition-to-plunge waveforms
• Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• Hydrodynamical constraints on bubble wall velocity
• Quasi-equilibrium configurations of binary systems of dark matter admixed neutron stars
• Full 3D Numerical Relativity Simulations of Neutron Star -- Boson Star Collisions with BAM
• High mass but low spin: an exclusion region to rule out hierarchical black-hole mergers as a mechanism to populate the pair-instability mass gap
• Interpreting the X-ray afterglows of gamma-ray bursts with radiative losses and millisecond magnetars
• Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals
• Gravitational wave inference on a numerical-relativity simulation of a black hole merger beyond general relativity
• The Energy Sources of Superluminous Supernovae
• The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
• Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
• Backreaction of axion-SU(2) dynamics during inflation
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• Detectability of QCD phase transitions in binary neutron star mergers: Bayesian inference with the next generation gravitational wave detectors
• The Dipole of the Astrophysical Gravitational-Wave Background
• Evolution of the Carter constant for a resonant inspiral into a Kerr black hole: I. The scalar case
• Self-consistent adiabatic inspiral and transition motion
• Frequency response of time-delay interferometry for space-based gravitational wave antennas
• Sharp turns in axion monodromy: primordial black holes and gravitational waves
• Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods
• Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
• Probing neutrino interactions and dark radiation with gravitational waves
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Gravitational waves from Population III binary black holes are consistent with LIGO/Virgo O3a data for the chirp mass larger than $\sim 20M_{\odot }$
• The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
• Gravitational smoothing of kinks on cosmic string loops
• Binary intermediate-mass black hole mergers in globular clusters
• Evolutionary Models for 15 Galactic Supernova Remnants with New Distances
• Axion clouds may survive the perturbative tidal interaction over the early inspiral phase of black hole binaries
• Multiband gravitational wave cosmology with stellar origin black hole binaries
• Hadron matter in neutron stars in view of gravitational wave observations
• Towards a unified treatment of gravitational-wave data analysis
• Eccentric Binary Black Holes with Spin via the Direct Integration of the Post-Newtonian Equations of Motion
• Impact of complex many-body correlations on electron capture in thermally excited nuclei around ${}^{78}$Ni
• Stability of domain walls in models with asymmetric potentials
• Millisecond Magnetars
• The scalar Green function of the Kerr spacetime
• On the detection and precise localisation of merging black holes events through strong gravitational lensing
• Influence of current mass on the spatially inhomogeneous chiral condensate
• Searching for scalar field dark matter with LIGO
• Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
• A note on the gravitational wave energy spectrum of parabolic and hyperbolic encounters
• Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence
• Exploring compact binary populations with the Einstein Telescope
• Gravitational back-reaction near cosmic string kinks and cusps
• Source Confusion from Neutron Star Binaries in Ground-Based Gravitational Wave Detectors is Minimal
• Methods and prospects for gravitational wave searches targeting ultralight vector boson clouds around known black holes
• Domain Wall Constraints on Two Higgs Doublet Models with $Z_2$ Symmetry
• Measuring tidal effects with the Einstein Telescope: A design study
• Gravitational-wave echoes from numerical-relativity waveforms via space-time construction near merging compact objects
• Gauge and Averaging in Gravitational Self-force
• The Gravitational Afterglow of Boson Stars
• Constraining the Initial Primordial Black Hole Clustering with CMB-distortion
• Eccentric Binary Neutron Star Search Prospects for Cosmic Explorer
• Determination of new coefficients in the angular momentum and energy fluxes at infinity to 9PN for eccentric Schwarzschild extreme-mass-ratio inspirals using mode-by-mode fitting
• GRB 191019A: a short gamma-ray burst in disguise from the disk of an active galactic nucleus
• Electromagnetic outflows in a class of scalar-tensor theories: binary neutron star coalescence
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: I. Non-Locality in Time and Infra-Red Divergencies
• Distinguishing the nature of ''ambiguous'' merging systems hosting a neutron star: GW190425 in low-latency
• Inspiralling compact objects with generic deformations
• Population Synthesis of Accreting Neutron Stars Emitting Gravitational Waves
• Gravitational wave astronomy with radio galaxy surveys
• On the probability of the extremely lensed $z$=6.2 Earendel source being a Population~III star
• Measuring the ringdown scalar polarization of gravitational waves in Einstein scalar Gauss-Bonnet gravity
• Scalar perturbations from inflation in the presence of gauge fields
• Forecasts for Low Spin Black Hole Spectroscopy in Horndeski Gravity
• Emission of gravitational waves by superconducting cosmic strings
• Searching for Ultra-light Bosons and Constraining Black Hole Spin Distributions with Stellar Tidal Disruption Events
• Primordial Black Holes from Axion Domain Wall Collapse
• Well-posed Cauchy formulation for Einstein-æther theory
• Newton potential in deSitter braneworld
• Addressing the challenges of detecting time-overlapping compact binary coalescences
• Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
• Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters
• Population III star formation in an X-ray background: III. Periodic radiative feedback and luminosity induced by elliptical orbits
• Flexible mapping of ringdown amplitudes for nonprecessing binary black holes
• PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions
• Numerical black hole initial data and shadows in dynamical Chern-Simons gravity
• Tabulated Neutron Star Equations of State Modeled within the Chiral Mean Field Model
• Extremely efficient mergers of intermediate mass black hole binaries in nucleated dwarf galaxies
• Utilizing Gaussian mixture models in all-sky searches for short-duration gravitational wave bursts
• Slow evolution of the metric perturbation due to a quasicircular inspiral into a Schwarzschild black hole
• Stochastic processes for pulsar timing noise: fluctuations in the internal and external torques
• Gravitational waves from accretion-induced descalarization in massive scalar-tensor theory
• Supernovae from massive stars
• Primordial Black Holes and Gravitational Waves in Multi-Axion-Chern-Simons Inflation
• Limits on electromagnetic counterparts of gravitational wave-detected binary black hole mergers
• Quantum black hole spectroscopy: probing the quantum nature of the black hole area using LIGO-Virgo ringdown detections
• Signatures of Ultralight Bosons in Compact Binary Inspiral and Outspiral
• The short gamma-ray burst population in a quasi-universal jet scenario
• Gravitational waves from magnetically-induced thermal neutron star mountains
• Identifying the SN 2022acko progenitor with JWST
• Gravitational microlensing by dressed primordial black holes
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• Correlated 1-1000 Hz magnetic field fluctuations from lightning over earth-scale distances and their impact on gravitational wave searches
• Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State
• GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
• Solving the 56Ni puzzle of magnetar-powered broad-lined type Ic supernovae
• Nonlinear Evolution of Quadratic Gravity in 3+1 Dimensions
• Three approaches for the classification of protoneutron star oscillation modes
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• Projected constraints on the dispersion of gravitational waves using advanced ground- and space-based interferometers
• Deep Generative Models of Gravitational Waveforms via Conditional Autoencoder
• Gravitational Collider Physics via Pulsar-Black Hole Binaries II: Fine and Hyperfine Structures are Favored
• Cosmic archaeology with massive stellar black hole binaries
• Anisotropic crystal structure of magnetized neutron star crust
• A census of OBe stars in nearby metal-poor dwarf galaxies reveals a high fraction of extreme rotators
• Stacking Gravitational Wave Signals from Soft Gamma Repeater Bursts
• Analyzing Gravitational Waves with General Relativity
• Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search
• Experimental signatures of gravitational wave bursters
• Monotonicity of the cores of massive stars
• Scattering of point particles by black holes: gravitational radiation
• Degeneracy in Studying the Supranuclear Equation of State and Modified Gravity with Neutron Stars
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Numerical studies on core collapse supernova in self-interacting massive scalar-tensor gravity
• Adapting to noise distribution shifts in flow-based gravitational-wave inference
• Neutron Star$-$Neutron Star and Neutron Star$-$Black Hole Mergers: Multiband Observations and Early Warnings
• Signature of Non-uniform Area Quantization on Black Hole Echoes
• STEP Survey II: Structural Analysis of 170 star clusters in the SMC
• Black hole-neutron star mergers from triples II: the role of metallicity and spin-orbit misalignment
• A sparse representation of gravitational waves from precessing compact binaries
• Precursors of Supernovae from Mass Eruption: Prospects for Early Warning of Nearby Core-collapse Supernovae
• Self-forced inspirals with spin-orbit precession
• On chromonatural inflation in string theory
• Multivariate Regression Analysis of Gravitational Waves from Rotating Core Collapse
• A frequency resolved atlas of the sky in continuous gravitational waves
• Eccentric-orbit extreme-mass-ratio-inspiral radiation II: 1PN correction to leading-logarithm and subleading-logarithm flux sequences and the entire perturbative 4PN flux
• Parameter Estimation for Stellar-Origin Black Hole Mergers In LISA
• Gravitational radiation reaction
• Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
• Resonances in Extreme Mass-Ratio Inspirals: Asymptotic and Hyperasymptotic Analysis
• Analyzing clustering of astrophysical gravitational-wave sources: Luminosity-distance space distortions
• Late-Phase Spectropolarimetric Observations of Superluminous Supernova SN 2017egm to Probe the Geometry of the Inner Ejecta
• Remnant masses from 1D+ core-collapse supernovae simulations: bimodal neutron star mass distribution and black holes in the low-mass gap
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Generating transient noise artifacts in gravitational-wave detector data with generative adversarial networks
• Probing the speed of gravity with LVK, LISA, and joint observations
• Merger-Ringdown Consistency: A New Test of Strong Gravity using Deep Learning
• Tidal Love numbers and approximate universal relations for fermion soliton stars
• Gravitational-wave dark siren cosmology systematics from galaxy weighting
• Probing dipole radiation from binary neutron stars with ground-based laser-interferometer and atom-interferometer gravitational-wave observatories
• The induced surface tension contribution for the equation of state of neutron stars
• Parameter estimation methods for analyzing overlapping gravitational wave signals in the third-generation detector era
• Multipole moments and universal relations for scalarized neutron stars
• Gravitational wave constraints on planetary-mass primordial black holes using LIGO O3a data
• Vanishing of Quadratic Love Numbers of Schwarzschild Black Holes
• The Type IIn Supernova 2010bt: The Explosion of a Star in Outburst
• High-accuracy waveforms for black hole-neutron star systems with spinning black holes
• Echoes from backreacting exotic compact objects
• Parameter estimation of a two-component neutron star model with spin wandering
• Evolutions of Nearly Maximally Spinning Black Hole Binaries Using the Moving Puncture Approach
• Hamiltonian for tidal interactions in compact binary systems to next-to-next-to-leading post-Newtonian order
• Neutron Star Quantum Death by Small Black Holes
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Breaking Mirror Twin Hypercharge
• A covariant approach to relativistic large-eddy simulations: The fibration picture
• Modified gravitational wave propagation and the binary neutron star mass function
• H$\alpha$ Reverberation Mapping of the Intermediate-Mass Active Galactic Nucleus in NGC 4395
• Time-domain metric reconstruction for hyperbolic scattering
• Inverse-chirp signals and spontaneous scalarisation with self-interacting potentials in stellar collapse
• Constraints for stellar electron-capture rates on ${}^{86}$Kr via the ${}^{86}$Kr($t$,${}^3$He$+\gamma$)${}^{86}$Br reaction and the implications for core-collapse supernovae
• Metric perturbations of Kerr spacetime in Lorenz gauge: Circular equatorial orbits
• Impact of electron capture rates on nuclei far from stability on core-collapse supernovae
• Detailed Calculation of Primordial Black Hole Formation During First-Order Cosmological Phase Transitions
• Smooth equations of state for high-accuracy simulations of neutron star binaries
• Formation of low-spinning 100 Msun black holes
• Coherent Gravitational Waveforms and Memory from Cosmic String Loops
• Gravitational Waves from Black-Hole Encounters: Prospects for Ground- and Galaxy-Based Observatories
• Self-force from reconstructed metric perturbations: numerical implementation in Schwarzschild spacetime
• Gap Transients Interacting with Circumstellar Medium
• Detecting High-Energy Neutrino Minibursts from Local Supernovae with Multiple Neutrino Observatories
• Classification of the core-collapse supernova explosion mechanism with learned dictionaries
• Interpolation in waveform space: enhancing the accuracy of gravitational waveform families using numerical relativity
• Cooling of Neutron Stars admixed with Light Dark Matter: a case study
• Nucleosynthesis in Outflows from Black Hole-Neutron Star Merger Disks With Full GR$\nu$RMHD
• Fermion Soliton Stars with Asymmetric Vacua
• GWitchHunters: Machine Learning and citizen science to improve the performance of Gravitational Wave detector
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Black hole remnant of black hole-neutron star coalescing binaries with arbitrary black hole spin
• Entropy-limited hydrodynamics: a novel approach to relativistic hydrodynamics
• Using machine learning to parametrize postmerger signals from binary neutron stars
• Tidal interaction of a small black hole in the field of a large Kerr black hole
• Searching for exotic cores with binary neutron star inspirals
• Bulk viscosity from Urca processes: $npe\mu$ matter in the neutrino-transparent regime
• Prospects for multi-messenger extended emission from core-collapse supernovae in the Local Universe
• Circumbinary discs around merging stellar-mass black holes
• Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
• The observed number counts in luminosity distance space
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• Well-posedness of cubic Horndeski theories
• Effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Prospects for detecting transient quasi-monochromatic gravitational waves from glitching pulsars with current and future detectors
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• PLE$\nu$M: A global and distributed monitoring system of high-energy astrophysical neutrinos
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• Quantifying uncertainties in general relativistic magnetohydrodynamic codes
• Calculation of $\beta$-decay half-lives with Skyrme Hartree-Fock-Bogoliubov+$pn$-QRPA and isoscalar pairing strengths optimized by a Bayesian method
• Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
• A study of the agreement between binary neutron star ejecta models derived from numerical relativity simulations
• Searching for spin-2 ULDM with gravitational waves interferometers
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Gravitational radiation contributions to the two-body scattering angle
• Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals
• Secondary accretion of dark matter in intermediate mass-ratio inspirals: Dark-matter dynamics and gravitational-wave phase
• Unbound motion on a Schwarzschild background: Practical approaches to frequency domain computations
• Shell-model based study of the direct capture in neutron-rich nuclei
• Precision cosmology with primordial GW backgrounds in presence of astrophysical foregrounds
• Characterizing a supernova's Standing Accretion Shock Instability with neutrinos and gravitational waves
• Radiation from Global Topological Strings using Adaptive Mesh Refinement: Massive Modes
• Detection and estimation of the cosmic dipole with the Einstein Telescope and Cosmic Explorer
• New self-force method via elliptic partial differential equations for Kerr inspiral models
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Numerical modelling of bulk viscosity in neutron stars
• Gravitational self-force in scalar-tensor gravity
• Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
• Nonlocal-in-time effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Effective-action model for dynamical scalarization beyond the adiabatic approximation
• Rapid pre-merger localization of binary neutron stars in third generation gravitational wave detectors
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference
• Turbulence modelling in neutron star merger simulations
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Gravitational radiation reaction in compact binary systems: Contribution of the magnetic dipole-magnetic dipole interaction
• Spontaneous Scalarization as a New Core-Collapse Supernova Mechanism and its Multi-Messenger Signals
• Gravitational backreaction on a cosmic string: Formalism
• Gravitational waves from small spin-up and spin-down events of neutron stars
• Targeted search for the kinematic dipole of the gravitational-wave background
• Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors
• Synergy between ground and space based gravitational wave detectors II: Localisation
• Detectability of SASI activity in supernova neutrino signals
• Interpretable AI forecasting for numerical relativity waveforms of quasi-circular, spinning, non-precessing binary black hole mergers
• Analytic Waveforms for Eccentric Gravitational Wave Bursts
• Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources
• Estimating the core compactness of massive stars with Galactic supernova neutrinos
• Unraveling Cosmological Anisotropies within Stochastic Gravitational Wave Backgrounds
• Numerical relativity higher order gravitational waveforms of eccentric, spinning, non-precessing binary black hole mergers
• Quasi-Normal Modes of Hairy Scalar Tensor Black Holes: Odd Parity
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds
• Nuclear Weak Rates and Nuclear Weak Processes in Stars
• Dark matter and bubble nucleation in old neutron stars
• Systematic analysis of inner crust composition using the extended Thomas-Fermi approximation with pairing correlations
• Reconstructing Gravitational Wave Core-Collapse Supernova Signals with Dynamic Time Warping
• Self-forced gravitational waveforms for Extreme and Intermediate mass ratio inspirals
• Spinning compact binary dynamics and chameleon orbits
• Deep Learning Model on Gravitational Waveforms in Merging and Ringdown Phases of Binary Black Hole Coalescences
• Correlated 0.01Hz-40Hz seismic and Newtonian noise and its impact on future gravitational-wave detectors
• Mimicking alternatives to inflation with interacting spectator fields
• On Black Hole Area Quantization and Echoes
• Transition from inspiral to plunge into a highly spinning black hole
• Frequency-domain approach to self-force in hyperbolic scattering
• Electromagnetic fields in compact binaries: a post-Newtonian approach
• Time-domain metric reconstruction for self-force applications
• Quantum dust cores of black holes
• MOCCA-SURVEY Database II -- Properties of Intermediate Mass Black Holes escaping from star clusters
• Spinning compact binary inspiral: Independent variables and dynamically preserved spin configurations
• Radiation Reaction for Non-Spinning Bodies at 4.5PN in the Effective Field Theory Approach
• A Robust Test of the Existence of Primordial Black Holes in Galactic Dark Matter Halos
• Application of the Hilbert-Huang transform for analyzing standing-accretion-shock-instability induced gravitational waves in a core-collapse supernova
• New search pipeline for gravitational waves with higher-order modes using mode-by-mode filtering
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• Ripples in Spacetime from Broken Supersymmetry
• Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• Long-term gravitational wave asteroseismology of supernova: from core collapse to 20 seconds postbounce
• Elliptica: a new pseudo-spectral code for the construction of initial data
• Electromagnetic Emission from a Binary Black Hole Merger Remnant in Plasma: Field Alignment and Plasma Temperature
• Measuring the properties of $f-$mode oscillations of a protoneutron star by third generation gravitational-wave detectors
• The 6x2pt method: supernova velocities meet multiple tracers
• A critical review of RHIC experimental results
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Gravitational-Wave Searches for Cosmic String Cusps in Einstein Telescope Data using Deep Learning
• Adapted gauge to small mass ratio binary black hole evolutions
• Parameterized Post-Einsteinian Framework for Precessing Binaries
• Gravitational Waves from Axion Monodromy
• A Spitzer Survey for Dust-Obscured Supernovae
• Combining neutrino experimental light-curves for pointing to the next Galactic Core-Collapse Supernova
• Chiral effective field theory description of neutrino nucleon-nucleon Bremsstrahlung in supernova matter
• A scalable elliptic solver with task-based parallelism for the SpECTRE numerical relativity code
• Constraining extended cosmologies with GW$\times$LSS cross-correlations
• From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments
• Redshift evolution of primordial black hole merger rate
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Coset Cosmology
• Pre-Supernova Alert System for Super-Kamiokande
• Emergence hour-by-hour of $r$-process features in the kilonova AT2017gfo
• Gravitational radiation close to a black hole horizon: Waveform regularization and the out-going echo
• Improving the convergence order of binary neutron star merger simulations in the Baumgarte-Shapiro-Shibata-Nakamura formulation
• Maximum latent heat of neutron star matter independently of General Relativity
• Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
• Search for Long-duration Gravitational-wave Signals Associated with Magnetar Giant Flares
• Continuous Gravitational Waves: A New Window to Look for Heavy Non-annihilating Dark Matter
• Electroweak Phase Transition with a Double Well Done Doubly Well
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Non-linear effects in EMRI dynamics and their imprints on gravitational waves
• Finite-temperature electron-capture rates for neutron-rich nuclei around N=50 and effects on core-collapse supernovae simulations
• Gravitational radiation from thermal mountains on accreting neutron stars: sources of temperature non-axisymmetry
• Constraining the cosmic merger history of intermediate-mass black holes with gravitational wave detectors
• Reverse phase transitions in binary neutron-star systems with exotic-matter cores
• Extending black-hole remnant surrogate models to extreme mass ratios
• Testing gravity with gravitational wave friction and gravitational slip
• Effects of orbital precession on hyperbolic encounters
• Oscillation dynamics of scalarized neutron stars
• Tidal Deformability of Neutron Stars in Scalar-Tensor Theories of Gravity
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• Molecular Dynamics for Dense Matter
• General relativistic magnetized Bondi-Hoyle-Lyttleton accretion with a spin-field misalignment: Jet nutation, polarity reversals, and Magnus drag
• Small-scale clustering of Primordial Black Holes: cloud-in-cloud and exclusion effects
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Lower-mass-gap Black Holes in Dense Star Clusters
• Revisiting Metastable Cosmic String Breaking
• Opportunities and limits of lunar gravitational-wave detection
• Evidence for gravitational-wave dominated emission in the central engine of short GRB 200219A
• The Mass Ratio Distribution of Tertiary Induced Binary Black Hole Mergers
• Exploring Supernova Gravitational Waves with Machine Learning
• Convolutional neural network search for long-duration transient gravitational waves from glitching pulsars
• Large Primordial Fluctuations in Gravitational Waves from Phase Transitions
• Primordial Black Holes with QCD Color Charge
• Stellar-mass black-hole binaries in LISA: characteristics and complementarity with current-generation interferometers
• Glitching pulsars as gravitational wave sources
• Intermediate mass black holes in globular clusters: effects on jerks and jounces of millisecond pulsars
• Scalable inference with Autoregressive Neural Ratio Estimation
• Probabilistic Model for the Gravitational Wave Signal from Merging Black Holes
• End-to-end study of the home and genealogy of the first binary neutron star merger
• Signal Space in the Triangular Network of Einstein Telescope
• Novel directed search strategy to detect continuous gravitational waves from neutron stars in low- and high-eccentricity binary systems
• Implicit-explicit (IMEX) evolution of single black holes
• Radio Power from a Direct-Collapse Black Hole in CR7
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Mass Distribution and Maximum Mass of Neutron Stars: Effects of Orbital Inclination Angle
• Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
• Footprints of population III stars in the gravitational-wave background
• The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors
• Inferring physical properties of stellar collapse by third-generation gravitational-wave detectors
• Localization of binary neutron star mergers with a single Cosmic Explorer
• What if GW190425 did not produce a black hole promptly?
• Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
• Core-collapse supernova subtypes in luminous infrared galaxies
• Testing anisotropic Hubble expansion
• Compact objects in and beyond the Standard Model from non-perturbative vacuum scalarization
• Conservative (failed)-tail effects at the fifth post-Newtonian order
• Gravitational wave memory of compact binary coalescence in the presence of matter effects
• Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
• Tensor-Multi-Scalar Gravity: Equations of Motion to 2.5 post-Newtonian Order
• Learning orbital dynamics of binary black hole systems from gravitational wave measurements
• Improved Moving-Puncture Techniques for Compact Binary Simulations
• General-relativistic radiation transport scheme in Gmunu II: Implementation of novel microphysical library for neutrino radiation -- Weakhub
• Measurement of the Cross-Correlation Angular Power Spectrum Between the Stochastic Gravitational Wave Background and Galaxy Over-Density
• Power-law modulation of the scalar power spectrum from a heavy field with a monomial potential
• Binary black hole mergers from Population III star clusters
• Spin-Orbit Misalignments in Tertiary-Induced Black-Hole Binary Mergers: Theoretical Analysis
• Thermonuclear and Electron-Capture Supernovae from Stripped-Envelope Stars
• Magnetically confined mountains on accreting neutron stars with multipole magnetic fields
• Quantum metric for null separated events and spacetime atoms
• Anatomy of parameter-estimation biases in overlapping gravitational-wave signals
• Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
• How the super-Eddington regime affects black hole spin evolution in high-redshift galaxies
• Implementation of a GHZ-Teukolsky puncture scheme for gravitational self-force calculations
• NRPyElliptic: A Fast Hyperbolic Relaxation Elliptic Solver for Numerical Relativity, I: Conformally Flat, Binary Puncture Initial Data
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• Measuring neutron-star distances and properties with gravitational-wave parallax
• Numerical Inside View of Hypermassive Remnant Models for GW170817
• Search for Gravitational Waves from Scorpius X-1 in LIGO O3 Data With Corrected Orbital Ephemeris
• The orbital-decay test of general relativity to the 2% level with 6-year VLBA astrometry of the double neutron star PSR J1537+1155
• Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations
• Simulations of Extreme-Mass-Ratio Inspirals Using Pseudospectral Methods
• Tidal Deformability Doppelgangers: Implications of a low-density phase transition in the neutron star equation of state
• Null-stream veto for two co-located detectors: Implementation issues
• Minimum star-forming halo mass in axion cosmology
• Gravitational waves from neutron-star mountains
• Enhancing the significance of gravitational wave bursts through signal classification
• Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology
• Evolution of inspiralling neutron star binaries: effects of tidal interactions and orbital eccentricities
• Spinning compact binary inspiral II: Conservative angular dynamics
• Multipolar gravitational waveforms and ringdowns generated during the plunge from the innermost stable circular orbit into a Schwarzschild black hole
• Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
• A proposed deep sea Neutrino Observatory in the Nanhai
• Autoencoder-driven Spiral Representation Learning for Gravitational Wave Surrogate Modelling
• Simultaneous bounds on the gravitational dipole radiation and varying gravitational constant from compact binary inspirals
• Gravitational wave surrogates through automated machine learning
• Identifying modified theories of gravity using binary black-hole ringdowns
• Domain wall annihilation -- a QFT perspective
• Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
• Transition of EMRIs through resonance: corrections to higher order in the on-resonance flux modification
• Quantum Love
• Sensitivity of third-generation interferometers to extra polarizations in the Stochastic Gravitational Wave Background
• Multi-messenger prospects for black hole - neutron star mergers in the O4 and O5 runs
• Strong Field Scattering of Black Holes: Assessing Resummation Strategies
• Cubic neutrons
• Gravitational radiation from inspiralling compact binaries to N${}^3$LO in the Effective Field Theory approach
• Prospects for Direct Detection of Black Hole Formation in Neutron Star Mergers with Next-Generation Gravitational-Wave Detectors
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• Neutron stars meet constraints from high and low energy nuclear physics
• Evolutions of unequal mass, highly spinning black hole binaries
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• Inverse-Chirp Imprint of Gravitational Wave Signals in Scalar Tensor Theory
• An upper limit on the spins of merging binary black holes formed through binary evolution
• Minimal Length, Nuclear Matter, and Neutron Stars
• Bayesian inference for binary neutron star inspirals using a Hamiltonian Monte Carlo Algorithm
• Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
• Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
• Unveiling the Nature of Gravitational-Wave Emission in Core-collapse Supernovae with Perturbative Analysis
• Gravitational-wave background in bouncing models from semi-classical, quantum and string gravity
• Early release of the expanded atlas of the sky in continuous gravitational waves
• Direct mapping of tidal deformability to the iso-scalar and iso-vector nuclear matter parameters
• Compact binary systems in Einstein-Aether gravity: Direct integration of the relaxed field equations to 2.5 post-Newtonian order
• On the Role of Muons in Binary Neutron Star Mergers: First Simulations
• Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
• Gravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors
• Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Validating Prior-informed Fisher-matrix Analyses against GWTC Data
• Postmerger multimessenger analysis of binary neutron stars: Effect of the magnetic field strength and topology
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds
• Boltzmann equations for astrophysical Stochastic Gravitational Wave Backgrounds scattering off of massive objects
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• Implications for Cosmic Domain Walls from LIGO-Virgo First Three Observing Runs
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• Rapid localization of gravitational wave hosts with FIGARO
• Modified Urca neutrino emissivity at finite temperature
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• Formalism for power spectral density estimation for non-identical and correlated noise using the null channel in Einstein Telescope
• Testing Unification and Dark Matter with Gravitational Waves
• Eccentricity estimation from initial data for Numerical Relativity Simulations
• Cyclotron line signatures of thermal and magnetic mountains from accreting neutron stars
• Treatments and placebos for the pathologies of effective field theories
• Analysis of the subsolar-mass black hole candidate SSM200308 from the second part of the third observing run of Advanced LIGO-Virgo
• The Spectrum of Gravitational Waves from Annihilating Domain Walls
• On the response of the Einstein Telescope to Doppler anisotropies
• Quasi-universal relations in the context of future neutron star detections
• A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo
• Gravitational-wave event rates as a new probe for dark matter microphysics
• Constraining Palatini gravity with GR-independent equations of state for neutron stars
• Gravitational Wave Astrometry for Rapidly Rotating Neutron Stars and Estimation of Their Distances
• The proto-neutron star inner crust in a multi-component plasma approach
• Galaxy rotation favors prolate dark matter haloes
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• The impact of nuclear reactions on the neutron-star g-mode spectrum
• Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities
• Detectability of stochastic gravitational wave background from weakly hyperbolic encounters
• Witnessing History: Rates and Detectability of Naked-Eye Milky-Way Supernovae
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Great Balls of FIRE III: Modeling Black Hole Mergers from Massive Star Clusters in Simulations of Galaxies
• Constraining the onset density for the QCD phase transition with the neutrino signal from core-collapse supernovae
• Spherical dust collapse in bimetric relativity: Bimetric polytropes
• Axial perturbations of hairy black holes in generalised scalar-tensor theories
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Revealing Phase Transition in Dense Matter with Gravitational Wave Spectroscopy of Binary Neutron Star Mergers
• Formation and fate of low metallicity stars in IllustrisTNG50
• Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach
• Impact of Rotation on the Multimessenger Signatures of a Hadron-quark Phase Transition in Core-collapse Supernovae
• Regularized calculation of the retarded Green function in Schwarzschild spacetime
• Scalar emission from neutron star-black hole binaries in scalar-tensor theories with kinetic screening
• Efficient simulations of high-spin black holes with a new gauge
• Angular power spectra of anisotropic stochastic gravitational wave background: developing statistical methods and analyzing data from ground-based detectors
• Quasi-normal modes and Microscopic Structure of the Schwarzschild Black Hole
• Classical Love for Quantum Blackholes
• Asymmetric Dark Matter from Gravitational Waves
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Covariant BSSN formulation in bimetric relativity
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Cosmic string bursts in LISA
• Energy and Angle Dependence of Neutrino Scattering Rates in Proto-Neutron Star and Supernova Matter within Skyrme RPA
• The possible existence of Pop III NS-BH binary and its detectability
• Gravitational waves from glitch-induced f-mode oscillations in quark and neutron stars
• Worldtube excision method for intermediate-mass-ratio inspirals: scalar-field model in 3+1 dimensions
• Formation of metal-free binaries: Impact of H${}_2$ line cooling and CIE cooling
• BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
• Crystallization in single and multicomponent Neutron Star crusts
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• Strong magnetic fields and pasta phases revisited
• Parameter Estimation with Nonstationary Noise in Gravitational-wave Data
• Impact of overlapping signals on parameterized post-Newtonian coefficients in tests of gravity
• Problematic systematics in neutron-star merger simulations
• Joint Optimization of seismometer arrays for the cancellation of Newtonian noise from seismic body waves in the Einstein Telescope
• XKN: a Semi-analytic Framework for the Modelling of Kilonovae
• Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G
• Strange quark matter as dark matter: 40 years later, a reappraisal
• Where binary neutron stars merge: predictions from IllustrisTNG
• Applications of the close-limit approximation: horizonless compact objects and scalar fields
• False positives for gravitational lensing: the gravitational-wave perspective
• Can we discern millilensed gravitational-wave signals from signals produced by precessing binary black holes with ground-based detectors?
• Identifying thermal effects in neutron star merger remnants with model-agnostic waveform reconstructions and third-generation detectors
• Deep learning to detect gravitational waves from binary close encounters: Fast parameter estimation using normalizing flows
• A model-independent tripartite test of cosmic distance relations
• Formulating the r-mode problem for slowly rotating neutron stars
• Characteristic formulation of the Regge-Wheeler and Zerilli Green functions
• Forecasting the population properties of merging black holes
• High priority targets for transient gravitational waves from glitching pulsars
• An analytic approach to quasinormal modes for coupled linear systems
• Repeated Gravitational Wave Bursts from Cosmic Strings
• Simulating neutron stars with a flexible enthalpy-based equation of state parametrization in SpECTRE
• Rotational mixing in close binaries
• Magnification and evolution bias of transient sources: GWs and SNIa
• Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
• Precise peculiar velocities from gravitational waves accompanied by electromagnetic signals and cosmological applications
• On the Testability of the Quark-Hadron Transition Using Gravitational Waves From Merging Binary Neutron Stars
• Measuring spin in coalescing binaries of neutron stars showing double precursors
• Search for gravitational wave signals from known pulsars in LIGO-Virgo O3 data using the 5n-vector ensemble method
• The onset of stellar multiplicity in massive star formation: A search for low-mass companions of massive young stellar objects with $L^{\prime }$-band adaptive optics imaging
• Worldtube excision method for intermediate-mass-ratio inspirals: self-consistent evolution in a scalar-charge model
• Impact of gravitational waveform model systematics on the measurement of the Hubble constant
• Tidal Love numbers of gravitational atoms
• Determination of the angular momentum distribution of supernovae from gravitational wave observations
• Initial Data and Eccentricity Reduction Toolkit for Binary Black Hole Numerical Relativity Waveforms
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Implementation of a new weave-based search pipeline for continuous gravitational waves from known binary systems
• Impact of signal clusters in wide-band searches for continuous gravitational waves
• A Fisher matrix for gravitational-wave population inference
• Merger of a Neutron Star with a Black Hole: one-family vs. two-families scenario
• Impact of lensing of gravitational waves on the observed distribution of neutron star masses
• Optimizing the Placement of Numerical Relativity Simulations using a Mismatch Predicting Neural Network
• High-energy neutrino signatures from pulsar remnants of binary neutron-star mergers: coincident detection prospects with gravitational waves
• Nuclear matter from the ladder resummation in terms of the experimental nucleon-nucleon scattering amplitudes
• Likelihood for a Network of Gravitational-Wave Detectors with Correlated Noise
• Gravitational Wave Signatures of Gauged Baryon and Lepton Number
• Ridges in rotating neutron-star properties due to first order phase transitions
• Universal relations for quasinormal modes of neutron stars in $R^2$ gravity
• QCD Axion Strings or Seeds?
• Gravitational Wave emission in Binary Neutron Star early post-merger within a dark environment
• Deep-Learning Classification and Parameter Inference of Rotational Core-Collapse Supernovae
• Virialized equation of state for warm and dense stellar plasmas in proto-neutron stars and Supernova matter
• Ultralight dark matter searches with KAGRA gravitational wave telescope
• Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications
• Mass octupole and current quadrupole corrections to gravitational wave emission from close hyperbolic encounters
• Impact of weak lensing on bright standard siren analyses
• Simple, efficient method of calculating the Detweiler-Whiting singular field to very high order
• Probing intermediate scale Froggatt-Nielsen models at future gravitational wave observatories
• Covariant approach to relativistic large-eddy simulations: Lagrangian filtering
• The equation of state of neutron stars and the role of nuclear experiments
• Combining chirp mass, luminosity distance and sky localisation from gravitational wave events to detect the cosmic dipole
• Accelerating the standard siren method: Improved constraints on modified gravitational-wave propagation with future data
• Planck Limits on Cosmic String Tension Using Machine Learning
• Probing nontensorial gravitational waves with a next-generation ground-based detector network
• Extreme Mass-Ratio Binary Black Hole Merger: Characteristics of the Test-Particle Limit
• Multi-messenger observations in the Einstein Telescope era: binary neutron star and black hole - neutron star mergers
• Black Hole - Neutron Star Binary Mergers: The Imprint of Tidal Deformations and Debris
• Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
• A Hubble constant estimation with dark standard sirens and galaxy cluster catalogues
• Exploring the neutron star zoo: An observational review
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• Distinguishing compact objects in extreme-mass-ratio inspirals by gravitational waves
• General Relativistic Equilibrium Models of Magnetized Neutron Stars
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Tidal deformability of neutron stars with exotic particles within a density dependent relativistic mean field model in R-squared gravity
• Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT
• Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
• Numerical-relativity surrogate modeling with nearly extremal black-hole spins
• Absence of strong CP violation
• Fundamental and higher-order excited modes of radial oscillation of neutron stars for various types of cold nucleonic and hyperonic matter
• Gravitational wave signals from long lasting binary-single black hole encounters
• Impact of gravitational lensing on black hole mass function inference with third-generation gravitational wave detectors
• Log-periodic gravitational-wave background beyond Einstein gravity
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• Reconstructing the star formation rate for compact binary populations with the Einstein telescope
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• Confinement Bubble Wall Velocity via Quasiparticle Determination
• Impact of Population III stars on the astrophysical gravitational-wave background
• Discontinuous collocation methods and gravitational self-force applications
• Time-domain modelling of Extreme-Mass-Ratio Inspirals for the Laser Interferometer Space Antenna
• Role of particle diffusion in shaping the gravitational wave signal from neutron star inspirals
• Self-consistent treatment of thermal effects in neutron-star post-mergers: observational implications for third-generation gravitational-wave detectors
• Equation of State of Decompressed Quark Matter, and Observational Signatures of Quark-Star Mergers
• Improving agnostic searches of Gravitational Waves from Neutron Star instabilities using image filtering
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• Multiplicity in 5 Msun Stars
• Gravitational waves from sub-solar mass primordial black holes
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background