GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Abstract

On August 17, 2017 at 12:41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per $8.0\times 10^4$ years. We infer the component masses of the binary to be between 0.86 and 2.26 $M_{\odot }$, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17 to 1.60 $M_{\odot }$, with the total mass of the system $2.74_{-0.01}^{+0.04}{M}_{\odot }$. The source was localized within a sky region of 28 deg${}^2$ (90% probability) and had a luminosity distance of $40_{-14}^{+8}$ Mpc, the closest and most precisely localized gravitational-wave signal yet. The association with the gamma-ray burst GRB 170817A, detected by Fermi-GBM 1.7 s after the coalescence, corroborates the hypothesis of a neutron star merger and provides the first direct evidence of a link between these mergers and short gamma-ray bursts. Subsequent identification of transient counterparts across the electromagnetic spectrum in the same location further supports the interpretation of this event as a neutron star merger. This unprecedented joint gravitational and electromagnetic observation provides insight into astrophysics, dense matter, gravitation and cosmology.

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• Black Holes in $f(T,B)$ Gravity: Exact and Perturbed Solutions
• Bridging the Gap: Categorizing Gravitational-Wave Events at the Transition Between Neutron Stars and Black Holes
• Dark matter admixed neutron star properties in the light of X-ray pulse profile observations
• Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation
• An improved test of the strong equivalence principle with the pulsar in a triple star system
• Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993
• General relativistic treatment of $f$-mode oscillations of hyperonic stars
• Environmental Noise in Advanced LIGO Detectors
• Exploring Features in the Binary Black Hole Population
• A New Method to Observe Gravitational Waves emitted by Core Collapse Supernovae
• GeV emission from a compact binary merger
• A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond
• Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
• Gravitational waves from colliding vacuum bubbles in gauge theories
• Tidal Deformability of Dark Matter Admixed Neutron Stars
• Universal Relations for Neutron Star F-Mode and G-Mode Oscillations
• The critical role of nuclear heating rates, thermalization efficiencies and opacities for kilonova modelling and parameter inference
• Multi-messenger observations of binary neutron star mergers in the O4 run
• Biases in parameter estimation from overlapping gravitational-wave signals in the third generation detector era
• Accelerating parameter inference with graphics processing units
• The Second Love Number of Dark Compact Planets and Neutron Stars with Dark Matter
• Realistic Finite-Temperature Effects in Neutron Star Merger Simulations
• Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
• Gravitational wave cosmology with extreme mass-ratio inspirals
• Coalescence of black hole--neutron star binaries
• All-sky Search for Continuous Gravitational Waves from Isolated Neutron Stars in the Early O3 LIGO Data
• Cosmology and modified gravitational wave propagation from binary black hole population models
• Preparing the next gravitational million-body simulations: Evolution of single and binary stars in Nbody6++GPU, MOCCA and McLuster
• Constraining f(R) gravity in solar system, cosmology and binary pulsar systems
• 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
• Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation
• Topical Review: Greybody Factors and Quasinormal Modes for Black Holes in Various Theories -- Fingerprints of Invisibles
• Defining eccentricity for gravitational wave astronomy
• NICER X-ray Observations of Seven Nearby Rotation-Powered Millisecond Pulsars
• First Constraints on Nuclear Coupling of Axionlike Particles from the Binary Neutron Star Gravitational Wave Event GW170817
• Bosonic Dark Matter in Light of the NICER Precise Mass-Radius Measurements
• Revisiting the shadow of braneworld black holes
• Phase transitions in neutron stars and their links to gravitational waves
• A Pixelated Approach to Galaxy Catalogue Incompleteness: Improving the Dark Siren Measurement of the Hubble Constant
• Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity
• Holographic modeling of nuclear matter and neutron stars
• Perturbing the perturbed: Stability of quasinormal modes in presence of a positive cosmological constant
• The Present and Future of QCD
• Detecting Supermassive Black Hole-Induced Binary Eccentricity Oscillations with LISA
• A comparative study of host galaxy properties between Fast Radio Bursts and stellar transients
• Asteroids for $\mu$Hz gravitational-wave detection
• The ANTARES Astronomical Time-Domain Event Broker
• Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae
• Low Mass X-ray Binaries: The Effects of the Magnetic Braking Prescription
• Impact of the neutron star crust on the tidal polarizability
• On the possibility of GW190425 being a black hole--neutron star binary merger
• Constraining the dense matter equation-of-state with radio pulsars
• Symmetry energy investigation with pion production from Sn+Sn systems
• Constraining the magnetic field structure in collisionless relativistic shocks with a radio afterglow polarization upper limit in GW170817
• Constraints on the maximum mass of neutron stars with a quark core from GW170817 and NICER PSR J0030+0451 data
• Linear Response, Hamiltonian and Radiative Spinning Two-Body Dynamics
• MLGWSC-1: The first Machine Learning Gravitational-Wave Search Mock Data Challenge
• Relativistic hypernuclear compact stars with calibrated equations of state
• Gravitational Wave Signal for Quark Matter with Realistic Phase Transition
• Ain't No Mountain High Enough: Semi-Parametric Modeling of LIGO-Virgos Binary Black Hole Mass Distribution
• Searches for Neutrinos from Gamma-Ray Bursts using the IceCube Neutrino Observatory
• Broad search for gravitational waves from subsolar-mass binaries through LIGO and Virgo's third observing run
• Quark-nuclear hybrid equation of state for neutron stars under modern observational constraints
• Extended calculations of energy levels and transition rates of Nd II-IV ions for application to neutron star mergers
• First demonstration of early warning gravitational wave alerts
• Insight-HXMT observations of the first binary neutron star merger GW170817
• Spectral Puzzle of the Off-Axis Gamma-Ray Burst in GW170817
• TeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• Perturbative QCD and the Neutron Star Equation of State
• The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425
• Neutron Star Mergers in AGN Accretion Disks: Cocoon and Ejecta Shock Breakouts
• Plausible presence of new state in neutron stars with masses above $0.98M_{\mathrm{TOV}}$
• Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
• When the entropy has no maximum: A new perspective on the instability of the first-order theories of dissipation
• Dependence of Gravitational Wave Transient Rates on Cosmic Star Formation and Metallicity Evolution History
• Black hole scalarization with Gauss-Bonnet and Ricci scalar couplings
• Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817
• The effects of self-interacting bosonic dark matter on neutron star properties
• Maximum mass of compact stars from gravitational wave events with finite-temperature equations of state
• Delta baryons and diquark formation in the cores of neutron stars
• Dark Matter or Regular Matter in Neutron Stars? How to tell the difference from the coalescence of compact objects
• Can neutron star mergers alone explain the r-process enrichment of the Milky Way?
• Investigating Signatures of Phase Transitions in Neutron-Star Cores
• SN2019dge: a Helium-rich Ultra-Stripped Envelope Supernova
• Radiation reaction for spinning black-hole scattering
• Measuring the eccentricity of GW170817 and GW190425
• Hyperspectral Pixel Unmixing with Latent Dirichlet Variational Autoencoder
• Impact of Dynamical Tides on the Reconstruction of the Neutron Star Equation of State
• Quasi-universal behaviour of the threshold mass in unequal-mass, spinning binary neutron-star mergers
• Asymmetric mass ratios for bright double neutron-star mergers
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• Gamma-Ray Bursts, Quasars, Baryonic Acoustic Oscillations, and Supernovae Ia: new statistical insights and cosmological constraints
• Neural networks reconstruction of the dense-matter equation of state from neutron-star parameters
• GW170817/GRB 170817A/AT2017gfo association: some implications for physics and astrophysics
• Closing a spontaneous-scalarization window with binary pulsars
• High Precision Ringdown Modeling: Multimode Fits and BMS Frames
• Emergence of microphysical bulk viscosity in binary neutron star post-merger dynamics
• Merger of two neutron stars: predictions from the two-families scenario
• Effect of hyperons on f-mode oscillations in Neutron Stars
• Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries
• Enhancing modified gravity detection from gravitational-wave observations using the Parametrized ringdown spin expansion coefficients formalism
• Detecting single gravitons with quantum sensing
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• Detection and Parameter Estimation of Gravitational Waves from Binary Neutron-Star Mergers in Real LIGO Data using Deep Learning
• Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
• LIGO Detector Characterization in the first half of the fourth Observing run
• Forecasting constraints on deviations from general relativity in $f(Q)$ gravity with standard sirens
• Virgo Detector Characterization and Data Quality: results from the O3 run
• Primordial black holes and secondary gravitational waves from natural inflation
• Multimessenger Constraints on Radiatively Decaying Axions from GW170817
• Evaporation of Primordial Black Holes in the Early Universe: Mass and Spin Distributions
• Gravitational bremsstrahlung from spinning binaries in the post-Minkowskian expansion
• Kilonova Detectability with Wide-Field Instruments
• g-mode Oscillations in Hybrid Stars: A Tale of Two Sounds
• Black hole-neutron star mergers are unlikely multi-messenger sources
• Modelling frequency-dependent tidal deformability for environmental black-hole mergers
• Thermodynamics and Shadows of GUP-corrected Black Holes with Topological Defects in Bumblebee Gravity
• Long-term evolution of neutron-star merger remnants in general relativistic resistive-magnetohydrodynamics with a mean-field dynamo term
• Modeling compact binary signals and instrumental glitches in gravitational wave data
• Dark degeneracy I: Dynamical or interacting dark energy?
• Uncertainty limits on neutron star radius measurements with gravitational waves
• Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger
• New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
• $f(R)$-gravity after the detection of the orbital precession of the S2 star around the Galactic centre massive black hole
• Binary Stars in the New Millennium
• A black hole detected in the young massive LMC cluster NGC 1850
• Static neutral black holes in Kalb-Ramond gravity
• How to assess the primordial origin of single gravitational-wave events with mass, spin, eccentricity, and deformability measurements
• Post-Minkowskian Radial Action from Soft Limits and Velocity Cuts
• The formation rate of short gamma-ray bursts and gravitational waves
• Second release of the CoRe database of binary neutron star merger waveforms
• Equation of state of dense matter in the multimessenger era
• On Primordial Black Holes and secondary gravitational waves generated from inflation with solo/multi-bumpy potential
• Nuclear Dynamics and Reactions in the Ab Initio Symmetry-Adapted Framework
• A brief overview of black hole-neutron star mergers
• Grids of stellar models with rotation: V. Models from 1.7 to 120 Msun at zero metallicity
• What neutron stars tell about the hadron-quark phase transition: a Bayesian study
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Strongly Lensed Transient Sources: A Review
• Tests of Gravitational-Wave Birefringence with the Open Gravitational-Wave Catalog
• The 6th Post-Newtonian Potential Terms at $O(G_N^4)$
• Relativistic mean-field theories for neutron-star physics based on chiral effective field theory
• GRMHD simulations of neutron-star mergers with weak interactions: r-process nucleosynthesis and electromagnetic signatures of dynamical ejecta
• Electromagnetism and hidden vector fields in modified gravity theories: spontaneous and induced vectorization
• Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing run
• Constraints on the presence of platinum and gold in the spectra of the kilonova AT2017gfo
• Unified model for the LISA measurements and instrument simulations
• ALMA and GMRT constraints on the off-axis gamma-ray burst 170817A from the binary neutron star merger GW170817
• Impacts of dark matter on the $f$-mode oscillation of hyperon star
• The effect of $f(R,T)$ modified gravity on mass and radius of pulsar HerX1
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• Possible Causes of False General Relativity Violations in Gravitational Wave Observations
• The R-Process Alliance: Chemo-Dynamically Tagged Groups of Halo $r$-Process-Enhanced Stars Reveal a Shared Chemical-Evolution History
• Gravitational Wave Astronomy With TianQin
• Redback: A Bayesian inference software package for electromagnetic transients
• Hybrid equation of state approach in binary neutron-star merger simulations
• Dependence of outer boundary condition on protoneutron star asteroseismology with gravitational-wave signatures
• Effects of spin on magnetized binary neutron star mergers and jet launching
• Updated observing scenarios and multi-messenger implications for the International Gravitational-wave Network's O4 and O5
• Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae
• Generalized framework for testing gravity with gravitational-wave propagation. III. Future prospect
• Ranking Love numbers for the neutron star equation of state: The need for third-generation detectors
• GRB 221009A Afterglow from a Shallow Angular Structured Jet
• Probing the Effective Quantum Gravity via Quasinormal Modes and Shadows of Black Holes
• Positivity Bounds on Dark Energy: When Matter Matters
• Is GW190425 consistent with being a neutron star$-$black hole merger?
• Primordial black holes and scalar induced gravitational waves from the $E$ model with a Gauss-Bonnet term
• Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Distinguishing Tidal Disruption Events from Impostors
• Microscopic equation of state of hot nuclear matter for numerical relativity simulations
• Targeted large mass ratio numerical relativity surrogate waveform model for GW190814
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Gamma-ray bursts afterglow physics and the VHE domain
• Status and perspectives of Continuous Gravitational Wave searches
• The Delay Time of Gravitational Wave -- Gamma-Ray Burst Associations
• The Heraklion Extragalactic Catalogue (HECATE): a value-added galaxy catalogue for multi-messenger astrophysics
• Assessing the impact of transient orbital resonances
• Propagation of a Short GRB Jet in the Ejecta: Jet Launching Delay Time, Jet Structure, and GW170817/GRB 170817A
• Maximum mass cutoff in the neutron star mass distribution and the prospect of forming supramassive objects in the double neutron star mergers
• Implications of PREX-2 on the electric dipole polarizability of neutron rich nuclei
• Improved ranking statistics of the GstLAL inspiral search for compact binary coalescences
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Implications of the search for optical counterparts during the second part of the Advanced LIGO's and Advanced Virgo's third observing run: lessons learned for future follow-up observations
• Probing pre-Recombination Physics by the Cross-Correlation of Stochastic Gravitational Waves and CMB Anisotropies
• Propagation of Polar Gravitational Waves in f(R,T) Scenario
• Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model
• Tidal Deformability of Fermion-Boson Stars: Neutron Stars Admixed with Ultra-Light Dark Matter
• The MPIfR-MeerKAT Galactic Plane survey I -- System setup and early results
• Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Higgsless simulations of cosmological phase transitions and gravitational waves
• Gravitational wave constraints on Lorentz and parity violations in gravity: high-order spatial derivative cases
• Electron Capture Supernovae From Close Binary Systems
• Symmetry energy constraints from GW170817 and laboratory experiments
• Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
• Target of Opportunity Observations of Gravitational Wave Events with Vera C. Rubin Observatory
• Search for nonlinear memory from subsolar mass compact binary mergers
• Astrophysical constraints on compact objects in 4D Einstein-Gauss-Bonnet gravity
• Gravitational signatures of a non--commutative stable black hole
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Transients from ONe White-Dwarf - Neutron-Star/Black-Hole Mergers
• Equations of state for hot neutron stars -- II. The role of exotic particle degrees of freedom
• Cosmic-ray database update: ultra-high energy, ultra-heavy, and anti-nuclei cosmic-ray data (CRDB v4.0)
• QCD Equation of State at Finite Chemical Potentials for Relativistic Nuclear Collisions
• Fission fragment distributions and their impact on the r-process nucleosynthesis in neutron star mergers
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Black hole merger simulations in wave dark matter environments
• Bayesian inference of strange star equation of state using the GW170817 and GW190425 data
• Massive $\Delta$-resonance admixed hypernuclear stars with anti-kaon condensations
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• Hubble Space Telescope non-detection of PSR J2144-3933: the coldest known neutron star
• Invertible disformal transformations with higher derivatives
• Continued radio observations of GW170817 3.5 years post-merger
• Measuring the propagation speed of gravitational waves with LISA
• Thin Accretion Disk onto slowly rotating black holes in Einstein-Æther theory
• Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
• Nucleosynthesis and observation of the heaviest elements
• Constraints on the Nieh-Yan modified teleparallel gravity with gravitational waves
• Resolving The Peak Of The Black Hole Mass Spectrum
• Imprints of r-process heating on fall-back accretion: distinguishing black hole-neutron star from double neutron star mergers
• Thermal Effects in Binary Neutron Star Mergers
• Rotating hairy black holes and thermodynamics from gravitational decoupling
• Trends of Neutron Skins and Radii of Mirror Nuclei from First Principles
• GRAthena++: puncture evolutions on vertex-centered oct-tree AMR
• Generalized quasi-Keplerian solution for eccentric, non-spinning compact binaries at 4PN order and the associated IMR waveform
• Deep-Learning Continuous Gravitational Waves: Multiple detectors and realistic noise
• On the minimum radius of very massive neutron stars
• Neutrinos and nucleosynthesis of elements
• Modeling differential rotations of compact stars in equilibriums
• Neutrino emission from binary neutron star mergers: characterizing light curves and mean energies
• Universal relation for supernova gravitational waves
• Jet Launching from Binary Neutron Star Mergers: Incorporating Neutrino Transport and Magnetic Fields
• On the motion of hairy black holes in Einstein-Maxwell-dilaton theories
• Compact body in a tidal environment: New types of relativistic Love numbers, and a post-Newtonian operational definition for tidally induced multipole moments
• No evidence of kinetic screening in simulations of merging binary neutron stars beyond general relativity
• Bayesian model-selection of neutron star equation of state using multi-messenger observations
• Ready-to-use Fourier domain templates for compact binaries inspiraling along moderately eccentric orbits
• Hints of Modified Gravity in Cosmos and in the Lab?
• Gravity experiments with radio pulsars
• Gravitational Bremsstrahlung with tidal effects in the post-Minkowskian expansion
• Origin of neutron capture elements with the Gaia-ESO survey: the evolution of s- and r-process elements across the Milky Way
• Evidence for $\gtrsim 4$ Gyr timescales of neutron star mergers from Galactic archaeology
• Redshift Effects in Particle Production from Kerr Primordial Black Holes
• Comparison of post-Minkowskian and self-force expansions: Scattering in a scalar charge toy model
• Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity
• Electric and magnetic dipole strength in 112,114,116,118,120,124Sn
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
• Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
• Observable Features of GW170817 Kilonova Afterglow
• Updated universal relations for tidal deformabilities of neutron stars from phenomenological equations of state
• 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
• Testing General Relativity with Gravitational Waves: An Overview
• Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
• Kinetic screening in nonlinear stellar oscillations and gravitational collapse
• The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae
• Difference in proton radii of mirror nuclei as a possible surrogate for the neutron skin
• Real-time gravitational-wave inference for binary neutron stars using machine learning
• Constraining self-interacting fermionic dark matter in admixed neutron stars using multimessenger astronomy
• Tidal Love Numbers of Novel and Admixed Celestial Objects
• No Detectable Kilonova Counterpart is Expected for O3 Neutron Star-Black Hole Candidates
• Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Optimising gravitational waves follow-up using galaxies stellar mass
• Probing the nuclear equation of state from the existence of a $\sim 2.6M_{\odot }$ neutron star: the GW190814 puzzle
• Constraints on the maximum densities of neutron stars from postmerger gravitational waves with third-generation observations
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Universality of the turbulent magnetic field in hypermassive neutron stars produced by binary mergers
• Long-duration Gamma-ray Burst and Associated Kilonova Emission from Fast-spinning Black Hole--Neutron Star Mergers
• Constraints on primordial curvature spectrum from primordial black holes and scalar-induced gravitational waves
• Radial Oscillations of Dark Matter admixed Neutron Stars
• Measuring the Hubble Constant with a sample of kilonovae
• Role of vector self-interaction in Neutron Star properties
• First-order thermodynamics of Horndeski gravity
• Discovering gravitationally lensed gravitational waves: predicted rates, candidate selection, and localization with the Vera Rubin Observatory
• A Bayesian inference of relativistic mean-field model for neutron star matter from observation of NICER and GW170817/AT2017gfo
• Quasinormal Modes of Non-Linearly Charged Black Holes surrounded by a Cloud of Strings in Rastall Gravity
• Effects of dark matter on the in-spiral properties of the binary neutron stars
• Common-spectrum process versus cross-correlation for gravitational-wave searches using pulsar timing arrays
• Limits on the Electromagnetic Counterpart to S190814bv
• Quarkyonic stars with isospin-flavor asymmetry
• Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
• Quasinormal modes of massive scalar fields in four-dimensional wormholes: anomalous decay rate
• Impact of Rastall gravity on mass, radius and sound speed of the pulsar PSR J0740+6620
• Dark matter effects on tidal deformabilities and moment of inertia in a hadronic model with short-range correlations
• Neutron stars in $f(R,L_m,T)$ gravity
• Comprehensive study of compact stars with dark matter
• Hierarchical Inference of Binary Neutron Star Mass Distribution and Equation of State with Gravitational Waves
• Can the PREX-2 and CREX results be understood by relativistic mean-field models with the astrophysical constraints?
• Nonoscillatory gravitational quasinormal modes and telling tails for Schwarzschild-de Sitter black holes
• Dense and Hot QCD at Strong Coupling
• Scalar QED as a toy model for higher-order effects in classical gravitational scattering
• Primordial black holes and scalar-induced gravitational waves from the generalized Brans-Dicke theory
• Element abundance patterns in stars indicate fission of nuclei heavier than uranium
• Mirror Neutron Stars
• Bayesian nonparametric inference of neutron star equation of state via neural network
• Cosmology with Standard Sirens at Cosmic Noon
• Quark formation and phenomenology in binary neutron-star mergers using V-QCD
• Training Strategies for Deep Learning Gravitational-Wave Searches
• Dynamical ejecta synchrotron emission as possible contributor to the changing behaviour of GRB170817A
• Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
• Astrophysical implications on hyperon couplings and hyperon star properties with relativistic equations of states
• Accuracy of relativistic Cowling approximation in protoneutron star asteroseismology
• Momentum Shell in Quarkyonic Matter from Explicit Duality: A Dual Model for Cold, Dense QCD
• Non-Gaussianity and Secondary Gravitational Waves from Primordial Black Holes Production in $\alpha$-attractor Inflation
• Search for gravitational waves from the coalescence of sub-solar mass and eccentric compact binaries
• Pure polarization test of GW170814 and GW170817 using waveforms consistent with modified theories of gravity
• Modelling neutron star mountains in relativity
• First-order phase transition and fate of false vacuum remnants
• Constraints on planetary and asteroid-mass primordial black holes from continuous gravitational-wave searches
• Optimising growth of structure constraints on modified gravity
• Strong lensing as a giant telescope to localize the host galaxy of gravitational wave event
• A simple parity violating model in the symmetric teleparallel gravity and its cosmological perturbations
• Observational Inference on the Delay Time Distribution of Short Gamma-ray Bursts
• Estimating outflow masses and velocities in merger simulations: impact of r-process heating and neutrino cooling
• GRB 211227A as a peculiar long gamma-ray burst from compact star merger
• GRB 211211A: a Neutron Star$-$White Dwarf Merger?
• General-relativistic hydrodynamics of non-perfect fluids: 3+1 conservative formulation and application to viscous black-hole accretion
• Gravitational perturbations of non-singular black holes in conformal gravity
• On the nature of the mass-gap object in the GW190814 event
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817
• Peaks of sound velocity in two color dense QCD: quark saturation effects and semishort range correlations
• Constructing Binary Neutron Star Initial Data with High Spins, High Compactness, and High Mass-Ratios
• Frequency deviations in universal relations of isolated neutron stars and postmerger remnants
• Constraining extra dimensions using observations of black hole quasi-normal modes
• Hunting extra dimensions in the shadow of Sgr A*
• Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
• Convolutional neural networks for the detection of the early inspiral of a gravitational-wave signal
• Light rings and long-lived modes in quasi-black hole spacetimes
• Neutron stars with large quark cores
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Probing Kilonova Ejecta Properties Using a Catalog of Short Gamma-Ray Burst Observations
• EoS for hot neutron stars
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• The high-density equation of state in heavy-ion collisions: Constraints from proton flow
• Searching for Isotropic Stochastic Gravitational-Wave Background in the International Pulsar Timing Array Second Data Release
• Thermal evolution of relativistic hyperonic compact stars with calibrated equations of state
• The role of weak interactions in dynamic ejecta from binary neutron star mergers
• Opacity of the highly ionized lanthanides and the effect on the early kilonova
• Alternative LISA-TAIJI networks
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• Nucleonic metamodelling in light of multimessenger, PREX-II and CREX data
• Separating Astrophysics and Geometry in Black Hole Images
• Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens
• Impact of the wave-like nature of Proca stars on their gravitational-wave emission
• Eikonal quasinormal modes of black holes beyond general relativity III: scalar Gauss-Bonnet gravity
• Analog Schwarzschild black holes of Bose-Einstein condensates in a cavity: Quasinormal modes and quasibound states
• The onset of spontaneous scalarization in generalised scalar-tensor theories
• Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state
• Resolving Galactic binaries in LISA data using particle swarm optimization and cross-validation
• Abundances of disk and bulge giants from high-resolution optical spectra -- IV. Zr, La, Ce, Eu
• Frequency response of space-based interferometric gravitational-wave detectors
• Template Bank for Compact Binary Coalescence Searches in Gravitational Wave Data: A General Geometric Placement Algorithm
• Afterglows and Kilonovae Associated with Nearby Low-Luminosity Short-Duration Gamma-Ray Bursts: Application to GW170817/GRB170817A
• Primordial black holes and secondary gravitational waves from chaotic inflation
• Freezing-In Gravitational Waves
• Influence of the crust on the neutron star macrophysical quantities and universal relations
• Massive and charged scalar field in Kerr-Newman spacetime: Absorption and superradiance
• Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
• Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3
• Dark Matter Effects on the Compact Star Properties
• Investigating Dark Matter-Admixed Neutron Stars with NITR Equation of State in Light of PSR J0952-0607
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
• Probing neutron-star matter in the lab: similarities and differences between binary mergers and heavy-ion collisions
• 3D radiative transfer kilonova modelling for binary neutron star merger simulations
• Parametrized tests of post-Newtonian theory using principal component analysis
• Numerical relativity for Horndeski gravity
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Implicit correlations within phenomenological parametric models of the neutron star equation of state
• Neutron Stars with Baryon Number Violation, Probing Dark Sectors
• Enrichment in r-process elements from multiple distinct events in the early Draco dwarf spheroidal galaxy
• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
• Effective field theory for gravitational radiation in scalar-tensor gravity
• $R^p$ Attractors Static Neutron Star Phenomenology
• Measuring the delay time distribution of binary neutron stars. II. Using the redshift distribution from third-generation gravitational wave detectors network
• $g$-modes of neutron stars with hadron-to-quark crossover transitions
• Constraints on strong phase transitions in neutron stars
• Gravitational lensing of a Schwarzschild-like black hole in Kalb-Ramond gravity
• Exploring the sky localization and early warning capabilities of third generation gravitational wave detectors in three-detector network configurations
• Gravitational lensing by a black hole in effective loop quantum gravity
• Search for black hole hyperbolic encounters with gravitational wave detectors
• A Neutron Star is born
• Double Neutron Star Formation: Merger Times, Systemic Velocities, and Travel Distances
• Analytic models of the spectral properties of gravitational waves from neutron star merger remnants
• The B-type Binaries Characterisation Programme I. Orbital solutions for the 30 Doradus population
• Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history
• Pre-merger localization of compact-binary mergers with third generation observatories
• On matrix method for black hole quasinormal modes
• Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
• Interplay Between Neutrino Kicks and Hydrodynamic Kicks of Neutron Stars and Black Holes
• Colour-Flavour Locked Quark Stars in Light of the Compact Object in HESS J1731-347 and the GW190814 Event
• Constraining the Properties of the Thermonuclear Burst Oscillation Source XTE J1814-338 Through Pulse Profile Modelling
• An empirical limit on the kilonova rate from the DLT40 one day cadence Supernova Survey
• Dimension dependence of numerical simulations on gravitational waves from protoneutron stars
• Nonsingular black holes in nonlinear gravity coupled to Euler-Heisenberg electrodynamics
• 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
• Actinide opacities for modeling the spectra and light curves of kilonovae
• Dynamical ejecta of neutron star mergers with nucleonic weak processes II: Kilonova emission
• A data-driven Reconstruction of Horndeski gravity via the Gaussian processes
• Linking the rates of neutron star binaries and short gamma-ray bursts
• Heavy double neutron stars: birth, mid-life and death
• Exploring the NANOGrav Signal and Planet-mass Primordial Black Holes through Higgs Inflation
• Malaise and remedy of binary boson-star initial data
• GW170817A as a Hierarchical Black Hole Merger
• Bulk viscosity from Urca processes: $npe\mu$ matter in the neutrino-trapped regime
• Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials
• A Fast Radio Burst discovered in FAST drift scan survey
• Using Deep Learning to Localize Gravitational Wave Sources
• Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3b
• Gaia pulsars and where to find them
• Vanishing Love of Black Holes in General Relativity: From Spacetime Conformal Symmetry of a Two-dimensional Reduced Geometry
• Hamiltonian analysis of mimetic scalar gravity revisited
• QCD phase diagram in a magnetized medium from the chiral symmetry perspective: The linear sigma model with quarks and the Nambu--Jona-Lasinio model effective descriptions
• Thermodynamics of Neutrons in a Magnetic Field and its Implications for Neutron Stars
• Luminosity-duration relations and luminosity functions of repeating and non-repeating fast radio bursts
• Constraints on the phase transition and nuclear symmetry parameters from PSR $\mathrm{J}0740+6620$ and multimessenger data of other neutron stars
• Rotating black holes in Einstein-aether theory
• The wide-field infrared transient explorer (WINTER)
• The wave nature of continuous gravitational waves from microlensing
• Primordial black holes and secondary gravitational waves from string inspired general no-scale supergravity
• Transient-optimised real-bogus classification with Bayesian Convolutional Neural Networks -- sifting the GOTO candidate stream
• Late time kilonova light curves and implications to GW 170817
• Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects
• Universal Inflationary Attractors Implications on Static Neutron Stars
• Correspondence between quasinormal modes and grey-body factors for massive fields in Schwarzschild-de Sitter spacetime
• Third post-Newtonian effective-one-body Hamiltonian in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• Universal relations for rapidly rotating cold and hot hybrid star
• Scattering of gravitational waves off spinning compact objects with an effective worldline theory
• Generalized disformal Horndeski theories: cosmological perturbations and consistent matter coupling
• On the diversity of magnetar-driven kilonovae
• New binary pulsar constraints on Einstein-æther theory after GW170817
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• Limit on the population of repeating fast radio bursts from the ASKAP/CRAFT lat50 survey
• The Off-Shell Recursion for Gravity and the Classical Double Copy for currents
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding
• Probing the speed of scalar-induced gravitational waves with pulsar timing arrays
• Inflationary Attractors Predictions for Static Neutron Stars in the Mass-Gap Region
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• Rotating neutron stars with quark cores
• $I-$Love$-C$ relation for an anisotropic neutron star
• Stochastic gravitational wave background phenomenology in a pulsar timing array
• $\nu \text{bhlight}$: Radiation GRMHD for Neutrino-Driven Accretion Flows
• NANOGrav signal and LIGO-Virgo Primordial Black Holes from the Higgs field
• Nuclear charge radii of silicon isotopes
• New insights into nuclear physics and weak mixing angle using electroweak probes
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• Metal-poor stars observed with the automated planet finder telescope. I. Discovery of five carbon-enhanced metal-poor stars from LAMOST
• Exploring the GRB population: Robust afterglow modelling
• Neutron Stars in Scalar-tensor Gravity with Quartic Order Scalar Potential
• Improved deep learning techniques in gravitational-wave data analysis
• Calabi-Yau meets Gravity: A Calabi-Yau three-fold at fifth post-Minkowskian order
• Twin stars as probes of the nuclear equation of state: effects of rotation through the PSR J0952-0607 pulsar and constraints via the tidal deformability from the GW170817 event
• Testing Cosmic Distance-Duality Relation from Future Gravitational Wave Standard Sirens
• On black bounce space-times in non-linear electrodynamics
• Impact of noise transients on low latency gravitational-wave event localisation
• Constraining quark-hadron interface tension in the multi-messenger era
• Signatures of R-process Enrichment in Supernovae from Collapsars
• Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
• Early warning of coalescing neutron-star and neutron-star-black-hole binaries from nonstationary noise background using neural networks
• First application of mass measurement with the Rare-RI Ring reveals the solar r-process abundance trend at A=122 and A=123
• Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing binary black hole coalescence
• High accuracy post-Newtonian and numerical relativity comparisons involving higher modes for eccentric binary black holes and a dominant mode eccentric inspiral-merger-ringdown model
• Neutron stars with a crossover equation of state
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
• New Graviton Mass Bound from Binary Pulsars
• Observational Constraints in Metric-Affine Gravity
• Fundamental Symmetries and Spacetime Geometries in Gauge Theories of Gravity: Prospects for Unified Field Theories
• LEGWORK: A python package for computing the evolution and detectability of stellar-origin gravitational-wave sources with space-based detectors
• Holographic approach to compact stars and their binary mergers
• Moment of inertia of slowly rotating anisotropic neutron stars in $f(R,T)$ gravity
• Multimessenger tests of the weak equivalence principle from GW170817 and its electromagnetic counterparts
• Gravitational traces of bumblebee gravity in metric-affine formalism
• Asymptotic decay and quasinormal frequencies of scalar and Dirac fields around dilaton-de Sitter black holes
• Thermonuclear Explosions and Accretion-induced Collapses of White Dwarfs in Active Galactic Nucleus Accretion Disks
• New effective precession spin for modeling multimodal gravitational waveforms in the strong-field regime
• Spectral method for metric perturbations of black holes: Kerr background case in general relativity
• Neutron Star Crust Can Support A Large Ellipticity
• Statistical study of gamma-ray bursts with jet break feature in multi-wavelength afterglow emissions
• Perturbations and Quasinormal Modes of the Dirac Field in Effective Quantum Gravity
• Effects of nuclear symmetry energy and equation of state on neutron star properties
• Event rate predictions of strongly lensed gravitational waves with detector networks and more realistic templates
• Systematic study on the quark-hadron mixed phase in compact stars
• Dynamical tides in neutron stars: The impact of the crust
• Spectral Method for the Gravitational Perturbations of Black Holes: Schwarzschild Background Case
• The Adaptive Transient Hough method for long-duration gravitational wave transients
• Bounds on GUP parameters from GW150914 and GW190521
• Studying the onset of deconfinement with multi-messenger astronomy of neutron stars
• Gravitational waves in non-local gravity
• General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking
• Neutron star mergers as the astrophysical site of the r-process in the Milky Way and its satellite galaxies
• Determination of properties of protoneutron stars toward black hole formation via gravitational wave observations
• Exact rotating wormholes via Ehlers transformations
• A Late-Time Galaxy-Targeted Search for the Radio Counterpart of GW190814
• Intermediate Mass-Ratio Inspirals with Dark Matter Minispikes
• Stochastic Chemical Evolution of Radioactive Isotopes with a Monte Carlo Approach
• Formulating bulk viscosity for neutron star simulations
• Translating neutron star observations to nuclear symmetry energy via artificial neural networks
• Constraints on the ultralight scalar boson from Advanced LIGO and Advanced Virgo's first three observing runs using the stochastic gravitational-wave background
• UV completions, fixing the equations and nonlinearities in $k$-essence
• Observability of inflated companion stars after supernovae in massive binaries
• Quasinormal Modes from EFT of Black Hole Perturbations with Timelike Scalar Profile
• Probing internal dissipative processes of neutron stars with gravitational waves during the inspiral of neutron star binaries
• Atmospheric NLTE models for the spectroscopic analysis of blue stars with winds. V. Complete comoving frame transfer, and updated modeling of X-ray emission
• Static Neutron Stars Perspective of Quadratic and Induced Inflationary Attractor Scalar-tensor Theories
• The $3+1$ Formalism in the Geometric Trinity of Gravity
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• Gravitational-wave constraints on the GWTC-2 events by measuring the tidal deformability and the spin-induced quadrupole moment
• Relativistic effective action of dynamical gravitomagnetic tides for slowly rotating neutron stars
• Echoes of Compact Objects in Scalar-Tensor Theories of Gravity
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• Constraining the Stochastic Gravitational Wave Background with Photometric Surveys
• CSHINE for studies of HBT correlation in Heavy Ion Reactions
• Formation of mass gap objects in highly asymmetric mergers
• Tidal deformations of hybrid stars with sharp phase transitions and elastic crusts
• Cosmography using strongly lensed gravitational waves from binary black holes
• Minimally Modified Gravity fitting Planck data better than $\Lambda$CDM
• Implementation of advanced Riemann solvers in a neutrino-radiation magnetohydrodynamics code in numerical relativity and its application to a binary neutron star merger
• Wigner Function Tomography via Optical Parametric Amplification
• Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers
• Ringing of a black hole in a dark matter halo
• Sensitivity functions for space-borne gravitational wave detectors
• Prospects for multi-messenger detection of binary neutron star mergers in the fourth LIGO-Virgo-KAGRA observing run
• Bayesian Inference of the Dense Matter Equation of State built upon Covariant Density Functionals
• Quark Models and Radial Oscillations: Decoding the HESS J1731-347 Compact Object's Equation of State
• Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and $\mathbf{\gamma }$-Ray Bursts
• Multiband Gravitational Wave Parameter Estimation: A Study of Future Detectors
• Covariant density functional theory input for r-process simulations in actinides and superheavy nuclei: the ground state and fission properties
• Impact of extreme spins and mass ratios on the post-merger observables of high-mass binary neutron stars
• Consequences of neutron decay inside neutron stars
• FAST early pulsar discoveries: Effelsberg follow-up
• On the moment of inertia of PSR J0737-3039 A from LIGO/Virgo and NICER
• General relativistic dynamical tides in binary inspirals, without modes
• Dark matter component in hadronic models with short-range correlations
• Minimally modified gravity with an auxiliary constraint: a Hamiltonian construction
• Constraints on the curvature of nuclear symmetry energy from recent astronomical data within the KIDS framework
• Multi-messenger-Athena Synergy White Paper
• The Astro-Primordial Black Hole Merger Rates: a Reappraisal
• General relativistic smoothed particle hydrodynamics
• Quadratic-in-spin interactions at fifth post-Newtonian order probe new physics
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Apparent Superluminality of Lensed Gravitational Waves
• A model-agnostic analysis of hybrid stars with reactive interfaces
• Constraining gravitational wave propagation using pulsar timing array correlations
• Possible consistent model of parity violations in the symmetric teleparallel gravity
• Quasinormal modes and thermodynamic properties of GUP-corrected Schwarzschild black hole surrounded by quintessence
• GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
• Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter
• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• Resonant tides in binary neutron star mergers: analytical-numerical relativity study
• Multi-messenger model for the prompt emission from GRB 221009A
• Perturbations and quasi-normal modes of black holes with time-dependent scalar hair in shift-symmetric scalar-tensor theories
• Hairy rotating black holes in cubic Galileon theory
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• Angular Momentum Loss Due to Tidal Effects in the Post-Minkowskian Expansion
• The BlackGEM telescope array I: Overview
• Hadron-quark mixed phase in the quark-meson coupling model
• The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
• Quasi-5.5PN TaylorF2 approximant for compact binaries: point-mass phasing and impact on the tidal polarizability inference
• Traversable wormholes in beyond Horndeski theories
• Large Eddy Simulations of Magnetized Mergers of Neutron Stars with Neutrinos
• Exploring the distribution and impact of bosonic dark matter in neutron stars
• Multi-Messenger Physics with the Pierre Auger Observatory
• A new approach and code for spinning black holes in modified gravity
• Strong-field effects in massive scalar-tensor gravity for slowly spinning neutron stars and application to X-ray pulsar pulse profiles
• Finding the remnants of the Milky Way's last neutron star mergers
• Interacting $ud$ and $uds$ quark matter at finite densities and quark stars
• Tidal Love numbers of Proca stars
• GW170817 4.5 years after merger: Dynamical ejecta afterglow constraints
• Dancing in the dark: detecting a population of distant primordial black holes
• Detection and parameter estimation of binary neutron star merger remnants
• Constraining nucleosynthesis in neutrino-driven winds: observations, simulations and nuclear physics
• Non-Gaussian Stochastic Gravitational Waves from Phase Transitions
• Inferring the neutron star maximum mass and lower mass gap in neutron star-black hole systems with spin
• Discovery of Three Candidate Magnetar-powered Fast X-ray Transients from Chandra Archival Data
• Constraining equation of state groups from $g$-mode asteroseismology
• R-modes as a New Probe of Dark Matter in Neutron Stars
• Analysis of a regular black hole in Verlinde's gravity
• Optical follow-up of gravitational wave events during the second advanced LIGO/VIRGO observing run with the DLT40 Survey
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• Cosmography with next-generation gravitational wave detectors
• Fast neutrino flavor conversions in a supernova: Emergence, evolution, and effects
• Memory, Penrose Limits and the Geometry of Gravitational Shockwaves and Gyratons
• Empirical constraints on the high-density equation of state from multi-messenger observables
• Equation of State table with hyperon and antikaon for supernova and neutron star merger
• Nearly model-independent constraints on dense matter equation of state in a Bayesian approach
• Novel Model of an Ultra-stripped Supernova Progenitor of a Double Neutron Star
• Seeing-limited imaging sky surveys -- small vs. large telescopes
• Spectroscopic r-Process Abundance Retrieval for Kilonovae I: The Inferred Abundance Pattern of Early Emission from GW170817
• Electroweak Phase Transition and Gravitational Waves in the Type-II Seesaw Model
• Testing gravitational wave propagation with multiband detections
• Constraints on high density equation of state from maximum neutron star mass
• An exploration of an early gravity transition in light of cosmological tensions
• Tracker and scaling solutions in DHOST theories
• Inferring the maximum and minimum mass of merging neutron stars with gravitational waves
• Long-term 3D-MHD Simulations of Black Hole Accretion Disks formed in Neutron Star Mergers
• Refined clock-jitter reduction in the Sagnac-type time-delay interferometry combinations
• The Effect of Jet-Ejecta Interaction on the Viewing Angle Dependence of Kilonova Light Curves
• Holographic approach to transport in dense QCD matter
• PUSHing core-collapse supernovae to explosions in spherical symmetry V: Equation of state dependency of explosion properties, nucleosynthesis yields, and compact remnants
• Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo
• DDOTI Observations of Gravitational-Wave Sources Discovered in O3
• Phases of rotating baryonic matter: non-Abelian chiral soliton lattices, antiferro-isospin chains, and ferri/ferromagnetic magnetization
• Missing one-loop contributions in secondary gravitational waves
• On the screening mechanism in DHOST theories evading gravitational wave constraints
• Effects of Dark Matter on $f$-mode oscillations of Neutron Stars
• Post-Minkowskian Theory Meets the Spinning Effective-One-Body Approach for Two-Body Scattering
• Common-envelope Dynamics of a Stellar-mass Black Hole: General Relativistic Simulations
• Quasinormal modes and shadows of a new family of Ayón-Beato-Garc\'ıa black holes
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
• Tossing Black Hole Spin Axes
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• Lensing of Gravitational Waves as a Novel Probe of Graviton Mass
• Defeating stochasticity: coalescence timescales of massive black holes in galaxy mergers
• Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
• Evolution of the dipole polarizability in the stable tin isotope chain
• The R-Process Alliance: J1521-3538, a very metal-poor, extremely r-process-enhanced star with [Eu/Fe]=+2.2, and the class of r-III stars
• A dynamically discovered and characterized non-accreting neutron star -- M dwarf binary candidate
• Discovery of the optical afterglow and host galaxy of short GRB181123B at $z=1.754$: Implications for Delay Time Distributions
• Quasinormal modes of dilatonic Reissner-Nordström black holes
• Binary neutron star mergers as a probe of quark-hadron crossover equations of state
• Dark particle mass effects on neutron star properties from a short-range correlated hadronic model
• On Thermal Stability of Hairy Black Holes
• GW190521 formation via three-body encounters in young massive star clusters
• I-Love-Q Relations for Neutron Stars in dynamical Chern Simons Gravity
• Assessing the compact-binary merger candidates reported by the MBTA pipeline in the LIGO-Virgo O3 run: probability of astrophysical origin, classification, and associated uncertainties
• Population Properties of Gravitational-Wave Neutron Star--Black Hole Mergers
• Generalized Approach to Matched Filtering using Neural Networks
• Accessing the Single-Particle Structure of the Pygmy Dipole Resonance in ${}^{208}$Pb
• Tidal deformability of strange stars and the GW170817 event
• Search for gravitational waves from five low mass X-ray binaries in the second Advanced LIGO observing run with an improved hidden Markov model
• Cosmological perturbations in Gauss-Bonnet quasi-dilaton massive gravity
• Characterizing Earth gravity field fluctuations with the MIGA antenna for future Gravitational Wave detectors
• Gravito-magnetic resonance in the field of a gravitational wave
• High-Precision X-ray Timing of Three Millisecond Pulsars with NICER: Stability Estimates and Comparison with Radio
• Filling the Mass Gap: How Kilonova Observations can Unveil the Nature of the Compact Object Merging with the Neutron Star
• Leveraging gravitational-wave memory to distinguish neutron star--black hole binaries from black hole binaries
• Can fermion-boson stars reconcile multi-messenger observations of compact stars?
• Relativistic star perturbations in Horndeski theories with a gauge-ready formulation
• Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
• Feeble DM-SM Interaction via New Scalar and Vector Mediators in Rotating Neutron Stars
• Demographics of neutron stars in young massive and open clusters
• Phase diagram and compact stars in a holographic QCD model
• On networks of space-based gravitational-wave detectors
• Anisotropic Strange Stars in the Spotlight: Unveiling Constraints through Observational Data
• Inflationary Dynamics and Swampland Criteria for Modified Gauss-Bonnet Gravity Compatible with GW170817
• Stability and gravitational collapse of neutron stars with realistic equations of state
• Light-ray operators, detectors and gravitational event shapes
• A multi-wavelength analysis of a collection of short-duration GRBs observed between 2012-2015
• Rapid and Robust Parameter Inference for Binary Mergers
• The photometric variability of massive stars due to gravity waves excited by core convection
• Symmetric Teleparallel Horndeski Gravity
• Gravitational waves effects in a Lorentz-violating scenario
• Laser Frequency Noise in Next Generation Gravitational-Wave Detectors
• The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
• ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
• Heavy Magnetic Neutron Stars
• Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12
• Probing hybrid stars with gravitational waves via interfacial modes
• Warm dense matter and cooling of supernovae remnants
• Gravitational memory effects in Chern-Simons modified gravity
• Effects of $\varphi$-meson on properties of hyperon stars in density dependent relativistic mean field model
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• Insights on the peak in the speed of sound of ultradense matter
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Closure relations of Gamma Ray Bursts in high energy emission
• Light curve classification with recurrent neural networks for GOTO: dealing with imbalanced data
• Modelling the chemical evolution of Zr, La, Ce and Eu in the Galactic discs and bulge
• Inference-optimized AI and high performance computing for gravitational wave detection at scale
• Black holes with a nonconstant kinetic term in degenerate higher-order scalar tensor theories
• First Exploration of Neutron Shell Structure Below Lead and Beyond $\mathbf{N}=126$
• Doppler boosting the stochastic gravitational wave background
• Eccentricity of Long Inspiraling Compact Binaries Sheds Light on Dark Sirens
• Performance of the KAGRA detector during the first joint observation with GEO 600 (O3GK)
• Quasinormal modes of self-dual black holes in loop quantum gravity
• The First Short GRB Millimeter Afterglow: The Wide-Angled Jet of the Extremely Energetic SGRB 211106A
• Igniting weak interactions in neutron star postmerger accretion disks
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• Inspiral of a Spinning Black Hole--Magnetized Neutron Star Binary: Increasing Charge and Electromagnetic Emission
• Relativistic mean field model for ultra-compact low mass neutron star of HESS J1731-347
• Resolving Galactic binaries using a network of space-borne gravitational wave detectors
• Muons in the aftermath of neutron star mergers and their impact on trapped neutrinos
• Constraining Collapsar r-Process Models through Stellar Abundances
• Absorption by black hole remnants in metric-affine gravity
• Fast ejecta as a potential way to distinguish black holes from neutron stars in high-mass gravitational-wave events
• Neutron rich matter in heaven and on Earth
• Bright "Merger-nova" Emission Powered by Magnetic wind from a New-Born Black Hole
• Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
• Dark matter effects on the properties of neutron stars: compactness and tidal deformability
• First constraint on the dissipative tidal deformability of neutron stars
• Quasinormal modes of Kerr black holes using a spectral decomposition of the metric perturbations
• First Constraints on the Photon Coupling of Axion-like Particles from Multimessenger Studies of the Neutron Star Merger GW170817
• Ensemble of Deep Convolutional Neural Networks for real-time gravitational wave signal recognition
• AT2018kzr: the merger of an oxygen-neon white dwarf and a neutron star or black hole
• Starquakes in millisecond pulsars and gravitational waves emission
• Gravitational wave populations and cosmology with neural posterior estimation
• General cosmological perturbations in teleparallel gravity
• Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors
• Crustal magnetic fields do not lead to large magnetic-field amplifications in binary neutron-star mergers
• Short gamma-ray burst jet propagation in binary neutron star merger environments
• Can the GW190814 secondary component be a bosonic dark matter admixed compact star?
• Reconnection-powered fast radio transients from coalescing neutron star binaries
• Correlations of r-Process Elements in Very Metal-Poor Stars as Clues to their Nucleosynthesis Sites
• Head-on collisions of $\ell$-boson stars
• Constraining Nuclear Symmetry Energy with Multi-messenger Resonant Shattering Flares
• Strange stars in $f(\mathcal{R})$ gravity Palatini formalism and gravitational wave echoes from them
• Sub-threshold binary neutron star search in Advanced LIGO's first observing run
• Electromagnetic precursor flares from the late inspiral of neutron star binaries
• Testing $\Lambda$-Free f(Q) Cosmology
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• Identification and removal of non-Gaussian noise transients for gravitational wave searches
• Abundance Patterns of $\alpha$ and Neutron-capture Elements in the Helmi Stream
• Measuring the Speed of Gravitational Waves from the First and Second Observing Run of Advanced LIGO and Advanced Virgo
• Plebanski-Demianski solutions in Quadratic gravity with conformally coupled scalar fields
• Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity
• Classification of Teleparallel Horndeski Cosmology via Noether Symmetries
• From quantum gravity to gravitational waves through cosmic strings
• LSTM and CNN application for core-collapse supernova search in gravitational wave real data
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Hybrid stars in light of the HESS J1731-347 remnant and the PREX-II experiment
• A global numerical model of the prompt emission in short gamma-ray bursts
• Gamma-Ray Flashes from Dark Photons in Neutron Star Mergers
• Effect of isovector scalar meson on equation of state of dense matter within relativistic mean field model
• Probing elastic quark phases in hybrid stars with radius measurements
• Lanthanides or dust in kilonovae: lessons learned from GW170817
• Hunting the stochastic gravitational wave background in pulsar timing array cross correlations through theoretical uncertainty
• Axisymmetric models for neutron star merger remnants with realistic thermal and rotational profiles
• Correlations between charge radii differences of mirror nuclei and stellar observables
• Deep Learning with Quantized Neural Networks for Gravitational Wave Forecasting of Eccentric Compact Binary Coalescence
• Impact of systematic nuclear uncertainties on composition and decay heat of dynamical and disk ejecta in compact binary mergers
• $r$-process nucleosynthesis from compact binary mergers
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• Anisotropic cosmological models in Horndeski gravity
• GW190814 follow-up with the optical telescope MeerLICHT
• The Influence of Beta Decay Rates on r-Process Observables
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data
• Constraining the long-lived magnetar remnants in short gamma-ray bursts from late-time radio observations
• Exploration of co-sputtered Ta${}_2$O${}_5$-ZrO${}_2$ thin films for gravitational-wave detectors
• Solar mass black holes from neutron stars and bosonic dark matter
• Investigating tidal heating in neutron stars via gravitational Raman scattering
• Looking for extra dimensions in the observed quasi-periodic oscillations of black holes
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Neutron stars colliding with binary companions: formation of hypervelocity stars, pulsar planets, bumpy superluminous supernovae and Thorne-Żytkow objects
• Resonant Shattering Flares as Multimessenger Probes of the Nuclear Symmetry Energy
• Probing the cosmic opacity from Future Gravitational Wave Standard Sirens
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• Neutrino spin oscillations in external fields in curved spacetime
• The R-Process Alliance: Chemo-Dynamically Tagged Groups II. An Extended Sample of Halo $r$-Process-Enhanced Stars
• Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue
• Fermi gas and modified gravity
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Quasinormal modes, thermodynamics and shadow of black holes in Hu-Sawicki f(R) gravity theory
• Prospects of gravitational waves in the minimal left-right symmetric model
• Three-Body Effective Potential in General Relativity at Second Post-Minkowskian Order and Resulting Post-Newtonian Contributions
• Phase Transitions in Neutron Stars
• Impact of massive neutron star radii on the nature of phase transitions in dense matter
• r-Process Radioisotopes from Near-Earth Supernovae and Kilonovae
• Magnetized discs and photon rings around Yukawa-like black holes
• Bottom-Up Reconstruction of Viable GW170817 Compatible Einstein-Gauss-Bonnet Theories
• Constraints on compact binary merger evolution from spin-orbit misalignment in gravitational-wave observations
• Resonant Shattering Flares in Black Hole-Neutron Star and Binary Neutron Star Mergers
• Primordial Black Hole Merger Rate in Ellipsoidal-Collapse Dark Matter Halo Models
• Cooling of hypernuclear compact stars: Hartree-Fock models and high-density pairing
• High Energy Neutrinos from Choked Gamma-Ray Bursts in AGN Accretion Disks
• Eccentric Mergers in AGN Discs: Influence of the Supermassive Black-Hole on Three-body Interactions
• High Tide: A Systematic Search for Ellipsoidal Variables in ASAS-SN
• Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
• The impact of isomers on a kilonova associated with neutron star mergers
• Quasinormal Modes of Dilaton Black Holes: Analytic approximations
• Long-lived Quasinormal modes around regular black holes and wormholes in Covariant Effective Quantum Gravity
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• Atomic Interferometric Gravitational-wave Space Observatory (AIGSO)
• Polar modes and isospectrality of Ellis-Bronnikov wormholes
• Cocoon breakout and escape from the ejecta of neutron star mergers
• Learning how to surf: Reconstructing the propagation and origin of gravitational waves with Gaussian Processes
• Framework for phase transitions between the Maxwell and Gibbs constructions
• Jet Launching from Merging Magnetized Binary Neutron Stars with Realistic Equations of State
• Scalar-tensor mixed polarization search of gravitational waves
• Axions: From Magnetars and Neutron Star Mergers to Beam Dumps and BECs
• Multimessenger signals from black hole-neutron star mergers without significant tidal disruption
• Constraints on the electromagnetic counterpart of the Neutron Star Black Hole merger GW200115
• Pre-merger alert to detect the very-high-energy prompt emission from binary neutron-star mergers: Einstein Telescope and Cherenkov Telescope Array synergy
• Bayesian refinement of covariant energy density functionals
• Neutron stars as extreme laboratories for gravity tests
• The equation of state and radial oscillations of neutron stars
• Precessing magnetars as central engines in short gamma-ray bursts
• The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors
• Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO
• Thermal Relaxation of Dark Matter Admixed Neutron Star
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• Potential Gravitational-wave and Gamma-ray Multi-messenger Candidate from Oct. 30, 2015
• A comprehensive search for the radio counterpart of GW190814 with the Australian Square Kilometre Array Pathfinder
• Modified gravitational wave propagation with higher modes and its degeneracies with lensing
• Multi-messenger Approaches to Supermassive Black Hole Binary Detection and Parameter Estimation: Implications for Nanohertz Gravitational Wave Searches with Pulsar Timing Arrays
• Relativistic hybrid stars with sequential first-order phase transitions in light of multimessenger constraints
• A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits
• Collapsars as Sites of r-process Nucleosynthesis: Systematic Near-Infrared Follow-up of Type Ic-BL Supernovae
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Hybrid neutron stars in the mass-radius diagram
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• The Chern-Simons Caps for Rotating Black Holes
• Impact of bulk viscosity on the post-merger gravitational-wave signal from merging neutron stars
• Axial quasi-normal modes of scalarized neutron stars with massive self-interacting scalar field
• Linear stability of black holes with static scalar hair in full Horndeski theories: generic instabilities and surviving models
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Triaxially-deformed Freely-precessing Neutron Stars: Continuous electromagnetic and gravitational radiation
• How does the Earth's rotation affect predictions of gravitational wave strong lensing rates?
• Primordial black holes formation and secondary gravitational waves in nonminimal derivative coupling inflation
• Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals
• The impact of natal kicks on galactic r-process enrichment by neutron star mergers
• Structure in the speed of sound: from neutron stars to heavy-ion collisions
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• Detectability of QCD phase transitions in binary neutron star mergers: Bayesian inference with the next generation gravitational wave detectors
• GeV Signatures of Short Gamma-Ray Bursts in Active Galactic Nuclei
• Electromagnetic counterparts of binary neutron star mergers leading to a strongly magnetized long-lived remnant neutron star
• Quark stars with a unified interacting equation of state in regularized 4D Einstein-Gauss-Bonnet gravity
• Gravitational Faraday rotation of gravitational waves by a Kerr black hole
• Spatially covariant gravity: Perturbative analysis and field transformations
• Hadron-quark Pasta Phase in Massive Neutron Stars
• Upscattered Cocoon Emission in Short Gamma-ray Bursts as High-energy Gamma-ray Counterparts to Gravitational Waves
• Improved Fermi-GBM GRB localizations using BALROG
• Thermal behavior as indicator for hyperons in binary neutron star merger remnants
• Gravitational-Wave and X-ray Probes of the Neutron Star Equation of State
• Follow-up of astrophysical transients in real time with the IceCube Neutrino Observatory
• Variability, periodicity and contact binaries in WISE
• Echoes from braneworld wormholes
• Rotating dark matter admixed neutron stars
• Can we decipher the composition of the core of a neutron star?
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Geometric approach for the modified second generation time delay interferometry
• Measuring Individual Masses of Binary White Dwarfs with Space-based Gravitational-wave Interferometers
• Speed of sound constraints on maximally rotating neutron stars
• SPHINCS_BSSN: A general relativistic Smooth Particle Hydrodynamics code for dynamical spacetimes
• Binary neutron star merger simulations with hot microscopic equations of state
• ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors
• Positivity bounds from multiple vacua and their cosmological consequences
• Scalarized neutron stars in massive scalar-tensor gravity: X-ray pulsars and tidal deformability
• New self-consistent effective one-body theory for spinless binaries based on the post-Minkowskian approximation
• Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
• Generating enhanced parity-violating gravitational waves during inflation with violation of the null energy condition
• Minimal theory of massive gravity and constraints on the graviton mass
• Highly r-process enhanced stars in ultra-faint dwarf galaxies
• $\text{Hi-COLA}$: Fast, approximate simulations of structure formation in Horndeski gravity
• Astrophysical Gravitational-Wave Echoes from Galactic Nuclei
• Spin-orbit effects for compact binaries in scalar-tensor gravity
• Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
• The High Time Resolution Universe Pulsar Survey -- XVII. PSR J1325-6253, a low eccentricity double neutron star system from an ultra-stripped supernova
• Implications of the Conformal Constraint on Sound Speed on the Radius of PSR J0952-0607 within Rastall Gravity
• Stringy Running Vacuum Model and current Tensions in Cosmology
• The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions
• Real-Time Detection of Anomalies in Large-Scale Transient Surveys
• Neutron star mass formula with nuclear saturation parameters for asymmetric nuclear matter
• A flexible Gaussian process reconstruction method and the mass function of the coalescing binary black hole systems
• Direct measurement of the distribution of dark matter with strongly lensed gravitational waves
• Solution to the hyperon puzzle using dark matter
• Search for Gamma-Ray Bursts and Gravitational Wave Electromagnetic Counterparts with High Energy X-ray Telescope of \textit{Insight}-HXMT
• On the detection and precise localisation of merging black holes events through strong gravitational lensing
• Magnetospheres of black hole-neutron star binaries
• Hybrid stars are compatible with recent astrophysical observations
• Early Warnings of Binary Neutron Star Coalescence using the SPIIR Search
• Circular orbits and polarized images of charged particles orbiting Kerr black hole with a weak magnetic field
• Modelling a $2.5M_{\odot }$ Compact Star with Quark Matter
• Overtones of black holes via time-domain integration
• Gravitational wave echoes from compact stars in $f(\mathcal{R},T)$ gravity
• Constraining a relativistic mean field model using neutron star mass-radius measurements II: Hyperonic models
• How to detect the shortest-period binary pulsars in the era of LISA
• Measuring the viscosity of dark matter with strongly lensed gravitational waves
• Impact of natal kicks on merger rates and spin-orbit misalignments of black hole -- neutron star mergers
• Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
• Gamma-Ray Emission Produced by $r$-process Elements from Neutron Star Mergers
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Eccentric Binary Black Holes with Spin via the Direct Integration of the Post-Newtonian Equations of Motion
• Inspiral gravitational waveforms from compact binary systems in Horndeski gravity
• Gravitational wave constraints on spatial covariant gravities
• HARM3D+NUC: A new method for simulating the post-merger phase of binary neutron star mergers with GRMHD, tabulated EOS and neutrino leakage
• Chasing Super-Massive Black Hole merging events with $Athena$ and LISA
• Identification of Binary Neutron Star Mergers in Gravitational-Wave Data Using YOLO One-Shot Object Detection
• Cocoon cooling emission in neutron star mergers
• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects
• A search for radio emission from double-neutron star merger GW190425 using Apertif
• Well-tempered teleparallel Horndeski cosmology: a teleparallel variation to the cosmological constant problem
• Rapidly rotating neutron stars in $f(R,T)$ gravity
• Quasinormal modes of charged black holes in Asymptotically Safe Gravity
• The Population of Eccentric Binary Black Holes: Implications for mHz Gravitational Wave Experiments
• Tuning Advanced LIGO to kilohertz signals from neutron-star collisions
• Optimizing Cadences with Realistic Light Curve Filtering for Serendipitous Kilonova Discovery with Vera Rubin Observatory
• Oscillation Modes and Gravitational Waves from Strangeon Stars
• Eccentric Binary Neutron Star Search Prospects for Cosmic Explorer
• Modeling gravitational waves from exotic compact objects
• Measuring tidal effects with the Einstein Telescope: A design study
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• X-ray afterglows of Short gamma-ray bursts: Magnetar or Fireball?
• Cold Atom Quantum Simulator for Dilute Neutron Matter
• Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
• Study of eccentric binaries in Horndeski theory
• Nuclear Matter and Neutron Stars from Relativistic Brueckner-Hartree-Fock Theory
• Self-consistent Effective-one-body theory for spinless binaries based on post-Minkowskian approximation I: Hamiltonian and decoupled equation for ${\psi }_4^B$
• CREX- and PREX-II-motivated relativistic interactions and their implications for the bulk properties of nuclear matter and neutron stars
• Tidal Love Numbers from EFT of Black Hole Perturbations with Timelike Scalar Profile
• Neutron stars in massive scalar-Gauss-Bonnet gravity: Spherical structure and time-independent perturbations
• Holographic QCD in the NICER era
• Determination of the symmetry energy from the neutron star equation of state
• Neutron star scalarization with Gauss-Bonnet and Ricci scalar couplings
• Astrometric Effects of Gravitational Wave Backgrounds with non-Luminal Propagation Speeds
• Compact Star in General $F(R)$ Gravity: Inevitable Degeneracy Problem and Non-Integer Power Correction
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• Polarization Modes of Gravitational Waves in Palatini Horndeski theory
• Baryonic models of ultra-low-mass compact stars for the central compact object in HESS J1731-347
• Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115
• Ultracompact hybrid stars consistent with multimessenger astrophysics
• Successful Higgs inflation from combined nonminimal and derivative couplings
• Magnetohydrodynamic simulations of self-consistent rotating neutron stars with mixed poloidal and toroidal magnetic fields
• Thermodynamics and Optical Properties of Phantom AdS Black Holes in Massive Gravity
• Nanohertz Gravitational Wave Astronomy during the SKA Era: An InPTA perspective
• Metric-affine gravity effects on terrestrial (exo-)planets profiles
• BIFROST: simulating compact subsystems in star clusters using a hierarchical fourth-order forward symplectic integrator code
• Neutron Star Structure in the Presence of Nonminimally Coupled Scalar Fields
• On the properties of a newborn magnetar powering the X-ray transient CDF-S XT2
• Testing the phase transition parameters inside neutron stars with the production of protons and lambdas in relativistic heavy-ion collisions
• Complementary constraints on dark energy equation of state from strongly lensed gravitational wave
• Equation-of-state-insensitive measure of neutron star stiffness
• Stability of black holes with non-minimally coupled scalar hair to the Einstein tensor
• Pulsar revival in neutron star mergers: multi-messenger prospects for the discovery of pre-merger coherent radio emission
• The new discontinuous Galerkin methods based numerical relativity program Nmesh
• g-mode Oscillations in Neutron Stars with Hyperons
• Constant-roll inflation in the generalized SU(2) Proca theory
• Measuring the neutron star compactness and binding energy with supernova neutrinos
• Determine the Lorentz factor and the viewing angle of GRB 170817A
• White dwarf stars in modified gravity
• Equilibrium sequences of differentially rotating stars with post-merger-like rotational profiles
• Electrically charged strange stars with an interacting quark matter equation of state
• Universal relations for compact stars with heavy baryons
• AGILE Observations of the Gravitational-wave Source GW170817: Constraining Gamma-Ray Emission from a NS-NS Coalescence
• Black hole-neutron star coalescence: effects of the neutron star spin on jet launching and dynamical ejecta mass
• Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
• On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel
• Hyperonic neutron stars: reconciliation between nuclear properties and NICER and LIGO/VIRGO results
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• Addressing the challenges of detecting time-overlapping compact binary coalescences
• Signatures of regular black holes from the shadow of Sgr A* and M87*
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• Constraints on cosmic curvature with lensing time delays and gravitational waves
• Luminal Propagation of Gravitational Waves in Scalar-tensor Theories: The Case for Torsion
• Constraints on $f(Q)$ logarithmic model using gravitational wave standard sirens
• Establishing the Non-Primordial Origin of Black Hole-Neutron Star Mergers
• The R-Process Alliance: Discovery of a low-alpha, r-Process-Enhanced Metal-Poor Star in the Galactic Halo
• Symmetry energy effect on the secondary component of GW190814 as a neutron star
• Gravitational wave asteroseismology for low-mass neutron stars
• Slow evolution of the metric perturbation due to a quasicircular inspiral into a Schwarzschild black hole
• Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario
• Ghost instability in the teleparallel gravity model with parity violations
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Long-Term Simulations of Dynamical Ejecta: Homologous Expansion and Kilonova Properties
• Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA
• Gravitational waves from accretion-induced descalarization in massive scalar-tensor theory
• Could a slow stable hybrid star explain the central compact object in HESS~J1731-347?
• MAGIC detection of GRB 201216C at $z=1.1$
• Implications of a Simpson-Visser solution in Verlinde's framework
• Quasinormal modes, greybody factors and thermodynamics of four dimensional AdS black holes in Critical Gravity
• Quantifying Relevance in Learning and Inference
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Extreme r-process enhanced stars at high metallicity in Fornax
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Generating enhanced primordial GWs during inflation with intermittent violation of NEC and diminishment of GW propagating speed
• Improvement of the target sensitivity in DECIGO by optimizing its parameters for quantum noise including the effect of diffraction loss
• Constraining the Braking Index and Energy Partition of Magnetar spindown with {\em Swift}/XRT data
• Scalar Fields Near Compact Objects: Resummation versus UV Completion
• Searches for Ultra-High-Energy Photons at the Pierre Auger Observatory
• Strange Stars within Bosonic and Fermionic Admixed Dark Matter
• Solving the $H_0$ tension in $f(T)$ Gravity through Bayesian Machine Learning
• Trans-iron Ge, As, Se, and heavier elements in the dwarf metal-poor stars, HD~19445, HD~84937, HD~94028, HD~140283, and HD~160617
• A Gravitational Wave Detector for Post Merger Neutron Stars: Beyond the Quantum Loss Limit of Michelson Fabry Perot Interferometer
• External Inverse-Compton Emission Associated with Extended and Plateau Emission of Short Gamma-Ray Bursts: Application to GRB 160821B
• Detecting Lorentz Violations with Gravitational Waves from Black Hole Binaries
• Chiral condensates for neutron stars in hadron-quark crossover: from a parity doublet nucleon model to an NJL quark model
• Characterizing the breakdown of quasi-universality in the post-merger gravitational waves from binary neutron star mergers
• Gravitational wave echoes from interacting quark stars
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Degeneracy in Studying the Supranuclear Equation of State and Modified Gravity with Neutron Stars
• Relativistic Mean Field Model parameterizations in the light of GW170817, GW190814, and PSR J0740 + 6620
• Pasta properties of the neutron star within effective relativistic mean-field model
• Secular evolution of compact binaries revolving around a spinning massive black hole
• The Virgo O3 run and the impact of the environment
• Neutron star mass-radius constraints using the high-frequency QPOs of GRB 200415A
• Revisiting the maximum mass of differentially rotating neutron stars in general relativity: Übermassive stars with realistic equations of state
• Model of hybrid star with baryonic and strange quark matter in Tolman-Kuchowicz spacetime
• Estimate for the bulk viscosity of strongly coupled quark matter using perturbative QCD and holography
• Properties of the neutron star crust: Quantifying and correlating uncertainties with improved nuclear physics
• From Neutrino- to Photon-Cooled in Three Years: Can Fallback Accretion Explain the X-ray Excess in GW170817?
• Anisotropic Durgapal-Fuloria Neutron Stars in $f(\mathcal{R},{\mathrm{T}}^2)$ Gravity
• A theory of mass transfer in binary stars
• Neutron Star in Covariant $f(Q)$ gravity
• Gaussian Processes for Glitch-robust Gravitational-wave Astronomy
• Effective description of generalized disformal theories
• On the Neutron Star/Black Hole Mass Gap and Black Hole Searches
• Orbital effects on time delay interferometry for TianQin
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• A First Search for Prompt Radio Emission from a Gravitational-Wave Event
• Implication of GW170817 for cosmological bounces
• Neutron Star Mergers and Gamma-Ray Bursts: Stripping Model
• Search strategies for long gravitational-wave transients: hidden Markov model tracking and seedless clustering
• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• Future prospects on testing extensions to $\Lambda$CDM through the weak lensing of gravitational waves
• Neutron Star$-$Neutron Star and Neutron Star$-$Black Hole Mergers: Multiband Observations and Early Warnings
• Hadron resonance gas with van der Waals interactions
• Probing the Impact of WIMP Dark Matter on Universal Relations, GW170817 Posterior and Radial Oscillations
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• On the Angular Momentum Transport Efficiency within the Star Constrained from Gravitational-wave Observations
• Gravitational Radiation from hyperbolic encounters in the presence of dark matter
• Constraining Energy-Momentum-Squared Gravity by binary pulsar observations
• XTE J1814-338 as a dark matter admixed neutron star
• The Hadron-Quark Crossover in Neutron Star within Gaussian Process Regression Method
• A Comparative Study of Long and Short GRBs. II. A Multi-wavelength Method to distinguish Type II (massive star) and Type I (compact star) GRBs
• Orbital eccentricity in a neutron star - black hole merger
• Utilizing the null stream of the Einstein Telescope
• The payload of the Lunar Gravitational-wave Antenna
• The MBTA Pipeline for Detecting Compact Binary Coalescences in the Fourth LIGO-Virgo-KAGRA Observing Run
• Impacts of anomaly on nuclear and neutron star equation of state based on a parity doublet model
• Binary Dynamics from Worldline QFT for Scalar-QED
• Modelling Populations of Kilonovae
• Novel neutron decay mode inside neutron stars
• Perturbative deflection angle, gravitational lensing in the strong field limit and the black hole shadow
• Differential configurational entropy and the gravitational collapse of a kink
• Structured, relativistic jets driven by radiation
• Where is Love? Tidal deformability in the black hole compactness limit
• Parameter estimation of a two-component neutron star model with spin wandering
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Confronting a set of Skyrme and ${\chi }_{EFT}$ predictions for the crust of neutron stars
• jetsimpy: A Highly Efficient Hydrodynamic Code for Gamma-ray Burst Afterglow
• Addition of tabulated equation of state and neutrino leakage support to IllinoisGRMHD
• Nuclear pasta structures and symmetry energy
• Generating transient noise artifacts in gravitational-wave detector data with generative adversarial networks
• Oscillating magnetised hybrid stars under the magnifying glass of multi-messenger observations
• Model-independent constraints on cosmic curvature: implication from the future gravitational wave observation DECIGO
• High-accuracy waveforms for black hole-neutron star systems with spinning black holes
• Mergers of Equal-Mass Binaries with Compact Object Companions from Mass Transfer in Triple Star Systems
• Probing the speed of gravity with LVK, LISA, and joint observations
• Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories
• Eighteen Years of Kilonova Discoveries with Swift
• The Kitt Peak Electron Multiplying CCD demonstrator
• Core Collapse Supernova Explosions in Active Galactic Nucleus Accretion Disks
• Extragalactic Millimeter Transients in the Era of Next Generation CMB Surveys
• Convolutional Neural Networks for the classification of glitches in gravitational-wave data streams
• Crustal properties of a neutron star within an effective relativistic mean-field model
• Radial Oscillations in Neutron Stars with Delta Baryons
• Rescuing constraints on modified gravity using gravitational redshift in large-scale structure
• XTE J1814-338: A potential hybrid star candidate
• Regular Black Holes from Proper-Time flow in Quantum Gravity and their Quasinormal modes, Shadow and Hawking radiation
• Instrumental Tip-of-the-iceberg Effects on the Prompt Emission of Swift/BAT Gamma-ray Bursts
• Probing black holes in a dark matter spike of M87 using quasinormal modes
• New quasi-universal relations for static and rapid rotating neutron stars
• Gravitational waves from fast-spinning white dwarfs
• From quarks and gluons to color superconductivity at supranuclear densities
• Tidal Love numbers and approximate universal relations for fermion soliton stars
• Efficient Learning of Accurate Surrogates for Simulations of Complex Systems
• Gravitational-wave dark siren cosmology systematics from galaxy weighting
• Unmodelled Clustering Methods for Gravitational Wave Populations of Compact Binary Mergers
• A compact instrument for gamma-ray burst detection on a CubeSat platform I: Design drivers and expected performance
• Quantum corrected thermodynamics of nonlinearly charged BTZ black holes in massive gravity's rainbow
• Symmetry energy effects on the properties of hybrid stars
• A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run
• The Gamow Explorer: A gamma-ray burst observatory to study the high redshift universe and enable multi-messenger astrophysics
• Quantum corrections to the quasinormal modes of the Schwarzschild black hole
• Initial data for general relativistic simulations of multiple electrically charged black holes with linear and angular momenta
• Testing GR with the Gravitational Wave Inspiral Signal GW170817
• Of Harbingers and Higher Modes: Improved gravitational-wave early-warning of compact binary mergers
• Non-Singular Black Holes and mass inflation in modified gravity
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Binary fractions of G and K dwarf stars based on the Gaia EDR3 and LAMOST DR5: impacts of the chemical abundances
• Analysis of the neutron matter equation of state and the symmetry energy up to fourth order of chiral effective field theory
• Stability of Hairy Black Holes in Shift-Symmetric Scalar-Tensor Theories via the Effective Field Theory Approach
• Classification of the core-collapse supernova explosion mechanism with learned dictionaries
• A search for compact object companions to high mass function single-lined spectroscopic binaries in Gaia DR3
• On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences
• Rapid localization of gravitational wave sources from compact binary coalescences using deep learning
• Instability and no-hair paradigm in d-dimensional charged-AdS black holes
• GECAM Localization of High Energy Transients and the Systematic Error
• The shape of Scalar Gauss-Bonnet Gravity
• Converting the signal-recycling cavity into an unstable optomechanical filter to enhance the detection bandwidth of gravitational-wave detectors
• Neutron Stars Harboring a Primordial Black Hole: Maximum Survival Time
• Jupiter and jovian (exo)-planets in Palatini $f(\bar{R})$ gravity
• Conformally coupled theories and their deformed compact objects: from black holes, radiating spacetimes to eternal wormholes
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• More on the first-order thermodynamics of scalar-tensor and Horndeski gravity
• Models of binary neutron star remnants with tabulated equations of state
• Neutron-capture elements in dwarf galaxies I: Chemical clocks & the short timescale of the r-process
• Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy
• The "Giraffe": Discovery of a stripped red giant in an interacting binary with a $\sim 2M_{\odot }$ lower giant
• MRI turbulence in accretion discs at large magnetic Prandtl numbers
• High-accuracy simulations of highly spinning binary neutron star systems
• Constraints on parity and Lorentz violations in gravity from GWTC-3 through a parametrization of modified gravitational wave propagations
• General-Relativistic Hydrodynamics Simulation of a Neutron Star - Sub-Solar-Mass Black Hole Merger
• Interpolating Detailed Simulations of Kilonovae: Adaptive Learning and Parameter Inference Applications
• Discovery of one neutron star candidate from radial velocity monitoring
• The classical and quantum implications of the Raychaudhuri Equation in f(T)-gravity
• A compact instrument for gamma-ray burst detection on a CubeSat platform II: Detailed design, assembly and validation
• Neutron star matter based on a parity doublet model including the $a_0(980)$ meson
• A bright electromagnetic counterpart to extreme mass ratio inspirals
• Circularly polarized scalar induced gravitational waves from the Chern-Simons modified gravity
• Asteroseismology using quadrupolar f-modes revisited: breaking of universal relationships in the slow hadron-quark conversion scenario
• Large-Scale Atom Interferometry for Fundamental Physics
• Central Speed of Sound, Trace Anomaly and Observables of Neutron Stars from Perturbative Analyses of Scaled TOV Equations
• Neutron star properties with careful parameterization in the (axial)vector meson extended linear sigma model
• Odd-parity stability of black holes in Einstein-Aether gravity
• The Gravitational-wave Optical Transient Observer (GOTO)
• Cosmological acceleration
• Constraining neutron star properties with a new equation of state insensitive approach
• Ultracompact horizonless objects in order-reduced semiclassical gravity
• Constraints on the velocity of gravitational waves from NANOGrav 15-year data set
• Generalized uncertainty principle in resonant detectors of gravitational waves
• Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
• Search for 10--1000 GeV neutrinos from Gamma Ray Bursts with IceCube
• Hyperonic Neutron Star Matter in Light of GW170817
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Detector performance of the Gamma-ray Transient Monitor onboard DRO-A Satellite
• Using machine learning to parametrize postmerger signals from binary neutron stars
• Constraints from compact star observations on non-Newtonian gravity in strange stars based on a density dependent quark mass model
• Cosmology of Supercooled Universe
• Search for continuous gravitational waves from ten H.E.S.S. sources using a hidden Markov model
• Two steps forward and one step sideways: the propagation of relativistic jets in realistic binary neutron star merger ejecta
• Anisotropic $k$-essence
• Wave effect of gravitational waves intersected with a microlens field: a new algorithm and supplementary study
• Fluid nature constrains Horndeski gravity
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Gravitational Waveform and Polarization from Binary Black Hole Inspiral in Dynamical Chern-Simons Gravity: From Generation to Propagation
• Prospects for detecting exoplanets around double white dwarfs with LISA and Taiji
• Magnetar as Central Engine of Gamma-Ray Bursts: Central Engine-Jet Connection, Wind-Jet Energy Partition, and Origin of Some Ultra-Long Bursts
• Calibration of gamma-ray bursts luminosity correlations using gravitational waves as standard sirens
• Neutron Stars in frames of $R^2$-gravity and Gravitational Waves
• Solar System tests and chameleon effect in f (R) gravity
• Electromagnetic signals from the decay of free neutrons in the first hours of neutron star mergers
• PEXO: a global modeling framework for nanosecond timing, microsecond astrometry, and $\mu$m/s radial velocities
• Quasinormal Modes for Dynamical Black Holes
• Equation of state constraints from multi-messenger observations of neutron star mergers
• Search for Low-energy Electron Antineutrinos in KamLAND Associated with Gravitational Wave Events
• Shell-model based study of the direct capture in neutron-rich nuclei
• On the Binary-Neutron-Star Post-Merger Magnetar Origin of XRT 210423
• Quasi-universality of the magnetic deformation of neutron stars in general relativity and beyond
• Conserved charges in Chern-Simons modified theory and memory effects
• Hyperon bulk viscosity and $r$-modes of neutron stars
• Exploring the Small Mass Limit of Stationary Black Holes in Theories with Gauss-Bonnet Terms
• Observational constraint from the heaviest pulsar PSR J0952-0607 on the equation of state of dense matter in relativistic mean field model
• Skyrme crystals, nuclear matter and compact stars
• The MPIfR-MeerKAT Galactic Plane Survey II. The eccentric double neutron star system PSR J1208-5936 and a neutron star merger rate update
• A critical discussion on the $H_0$ tension
• Dynamical tides during the inspiral of rapidly spinning neutron stars: Solutions beyond mode resonance
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• Non-radial oscillations in anisotropic dark energy stars
• Unified neutron star equations of state calibrated to nuclear properties
• Gravitationally induced matter creation in scalar-tensor $f(R,T_{\mu \nu }{T}^{\mu \nu })$ gravity
• Primordial black holes in scalar field inflation coupled to the Gauss-Bonnet term with fractional power-law potentials
• Extending the Chemical Reach of the H3 Survey: Detailed Abundances of the Dwarf-galaxy Stellar Stream Wukong/LMS-1
• Tidal heating as a direct probe of strangeness inside neutron stars
• Superheavy Elements in Kilonovae
• The Large Array Survey Telescope -- Science Goals
• Constraining mass, radius and tidal deformability of compact stars with axial wI modes: new universal relations including slow stable hybrid stars
• Precision cosmology with primordial GW backgrounds in presence of astrophysical foregrounds
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• Characterizing a supernova's Standing Accretion Shock Instability with neutrinos and gravitational waves
• Quantifying uncertainties in general relativistic magnetohydrodynamic codes
• Constraining the equation of state of hybrid stars using recent information from multidisciplinary physics
• Phase transitions and resilience of the MDCDW phase at finite temperature and density
• Chemical Evolution of Ytterbium in the Galactic Disk
• A systematic study of super-Eddington layers in the envelopes of massive stars
• Gravitational waves from tidal disruption events: an open and comprehensive catalogue
• Understanding binary neutron star collisions with hypermodels
• Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Parameterized non-relativistic limit of stellar structure equations in Ricci-based gravity theories
• The I-Love-Q Relations for Superfluid Neutron Stars
• Density estimation with Gaussian processes for gravitational-wave posteriors
• Unbiased likelihood-free inference of the Hubble constant from light standard sirens
• Generalised gravitational burst generation with Generative Adversarial Networks
• Deep exploration for continuous gravitational waves at 171--172 Hz in LIGO second observing run data
• Combining cosmological and local bounds on bimetric theory
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• Microscopic nuclear equation of state at finite temperature and stellar stability
• Electromagnetic emission from axionic boson star collisions
• Influence of the treatment of initialization and mean-field potential on the neutron to proton yield ratios
• Prospects for kilonova signals in the gravitational-wave era
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Extended reduced-order surrogate models for scalar-tensor gravity in the strong field and applications to binary pulsars and gravitational waves
• Ghost and Laplacian Instabilities in the Teleparallel Horndeski Gravity
• Compactness in the Thermal Evolution of Twin Stars
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds
• Gravitational wave birefringence in spatially curved teleparallel cosmology
• Multiple measurements of gravitational waves acting as standard probes: model-independent constraints on the cosmic curvature with DECIGO
• $2.6M_{\odot }$ Compact Object and Neutron Stars within Eddington-Inspired Born-Infeld Theory of Gravity
• Neutron Stars in Scalar-Tensor Theories: Analytic Scalar Charges and Universal Relations
• Probing horizon scale quantum effects with Love
• Universal relations for rotating Boson Stars
• Rainbow scattering of gravitational plane waves by a compact body
• Relativistic approach for the determination of nuclear and neutron star properties in consideration of PREX-II results
• Hybrid stars with large strange quark cores constrained by GW170817
• Deciphering the unusual stellar progenitor of GRB 210704A
• Manifest colour-kinematics duality and double-copy in the string-based formalism
• Numerical modelling of bulk viscosity in neutron stars
• Induced Gravitational Waves from Multi-Sound Speed Resonances during Cosmological Inflation
• Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference
• Comparison between the Thomas-Fermi and Hartree-Fock-Bogoliubov Methods in the Inner Crust of a Neutron Star: The Role of Pairing Correlations
• Compact star merger events with stars composed of interacting strange quark matter
• Black hole formation in relativistic Oscillaton collisions
• Quasinormal modes, temperatures and greybody factors of black holes in a generalized Rastall gravity theory
• Exploring universal characteristics of neutron star matter with relativistic \textit{ab initio} equations of state
• Constraining the long-lived supramassive neutron stars by magnetar boosted kilonovae
• Inferring neutron star properties with continuous gravitational waves
• GAMMA: a new method for modeling relativistic hydrodynamics and non-thermal emission on a moving mesh
• Rapidly rotating neutron stars: Universal relations and EOS inference
• Magnetar QPOs and neutron star crust elasticity
• Jetlike structures in low-mass binary neutron star merger remnants
• Rapid pre-merger localization of binary neutron stars in third generation gravitational wave detectors
• Strangeness $S=-3$ and $-4$ baryon-baryon interactions in relativistic chiral effective field theory
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• Anisotropic multimessenger signals from black hole neutrino-dominated accretion flows with outflows in binary compact object mergers
• Stealth black holes in shift symmetric kinetic gravity braiding
• Impact of The Newly Revised Gravitational Redshift of X-ray Burster GS 1826-24 on The Equation of State of Supradense Neutron-Rich Matter
• Frequency planning for LISA
• What Powered the Kilonova-Like Emission After GRB 230307A in the Framework of a Neutron Star-White Dwarf Merger?
• Black hole quasinormal modes in the era of LIGO
• Stringent Pulsar Timing Bounds on Light Scalar Couplings to Matter
• Hot neutron stars and their equation of state
• Applying the effective-source approach to frequency-domain self-force calculations for eccentric orbits
• Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
• Probing neutron star structure via f-mode oscillations and damping in dynamical spacetime models
• Energy-dependent and energy-integrated two-moment general-relativistic neutrino transport simulations of hypermassive neutron star
• How the QCD trace anomaly behaves at the core of twin stars?
• Properties of neutron star described by a relativistic $abinitio$ model
• Neutron stars in the bumblebee theory of gravity
• Universal properties of maximum-mass neutron stars: a new tool to explore superdense matter
• Looking out for the Galileon in the nanohertz gravitational wave sky
• The Guided Moments formalism: a new efficient full-neutrino treatment for astrophysical simulations
• Needle in a Bayes Stack: a Hierarchical Bayesian Method for Constraining the Neutron Star Equation of State with an Ensemble of Binary Neutron Star Post-merger Remnants
• Jet-environment interplay in magnetized binary neutron star mergers
• Magnetic-Field Induced Deformation in Hybrid Stars
• A Robust Test of the Existence of Primordial Black Holes in Galactic Dark Matter Halos
• Towards Uncovering Dark Matter Effects on Neutron Star Properties: A Machine Learning Approach
• Convolutional neural network for gravitational-wave early alert: Going down in frequency
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Studies of the equation-of-state of nuclear matter by heavy-ion collisions at intermediate energy in the multi-messenger era
• Gravitational-wave polarizations in generic linear massive gravity and generic higher-curvature gravity
• Glitch subtraction from gravitational wave data using adaptive spline fitting
• Proca theory of four-dimensional regularized Gauss-Bonnet gravity and black holes with primary hair
• Gamma-Ray Bursts
• Testing the Speed of Gravity with Black Hole Ringdown
• GUP-corrected black holes: Thermodynamic properties, evaporation time and shadow constraint from EHT Observations of M87* and Sgr A*
• Electromagnetic fields in compact binaries: a post-Newtonian approach
• Speed of sound in dense matter and two families of compact stars
• Constraining DHOST theories with linear growth of matter density fluctuations
• Effect of nucleon effective mass and symmetry energy on the neutrino mean free path in a neutron star
• Selecting Horndeski theories without apparent symmetries and their black hole solutions
• Radiopurity of a kg-scale PbWO${}_4$ cryogenic detector produced from archaeological Pb for the RES-NOVA experiment
• Mass$\unicode{x2013}$spin Re-Parameterization for Rapid Parameter Estimation of Inspiral Gravitational-Wave Signals
• Propagation of scalar and tensor gravitational waves in Horndeski theory
• The future of gravitational theories in the era of the gravitational wave astronomy
• Constraining Horndeski theory with gravitational waves from coalescing binaries
• Predicting electromagnetic counterparts using low-latency, gravitational-wave data products
• GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins
• Parameterized Post-Einsteinian Framework for Precessing Binaries
• Resolving phase transition properties of dense matter through tidal-excited g-mode from inspiralling neutron stars
• Breaking of universal relationships of axial wI-modes in hybrid stars: rapid and slow hadron-quark conversion scenarios
• Nonparametric model for the equations of state of neutron star from deep neural network
• Quantum Skyrmion crystals and the symmetry energy of dense matter
• GRANDMA Observations of ZTF/Fink Transients during Summer 2021
• Fluid pulsation modes and tidal deformability of anisotropic strange stars in light of the GW$170817$ event
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• The Galactic Underworld: The spatial distribution of compact remnants
• Interacting Kilonovae: Long-lasting Electromagnetic Counterparts to Binary Mergers in the Accretion Disks of Active Galactic Nuclei
• Numerical Study of Stellar Core Collapse and Neutrino Emission Using the Nuclear Equation of State Obtained by the Variational Method
• Time Evolution of Black Hole Perturbations in Quadratic Gravity
• On Black Hole Area Quantization and Echoes
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• Fallback Accretion Model for the Years-to-Decades X-ray Counterpart to GW170817
• Evolution of equal mass binary bare quark stars in full general relativity: could a supramassive merger remnant experience prompt collapse?
• Multi-messenger Extended Emission from the compact remnant in GW170817
• Hybrid Strangeon Stars
• Probing hadron-quark phase transition in twin stars using $f$-modes
• Self-consistent MHD simulation of jet launching in a neutron star - white dwarf merger
• Implications of the fermion vacuum term in the extended SU(3) Quark Meson model on compact stars properties
• Rotating black hole in $f(R)$ theory
• GW190521 formation scenarios via relativistic accretion
• Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
• Gravitational atoms in the braneworld scenario
• Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories
• Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
• The sound of the event horizon
• Spherically symmetric exact vacuum solutions in Einstein-aether theory
• Spinning Particle Dynamics and ISCO in Covariant Loop Quantum Gravity
• Revisiting the Galactic Double Neutron Star merger and LIGO detection rates
• Exponentially Decaying Extended Emissions Following Short Gamma-Ray Bursts with Possible Luminosity -- E-folding Time Correlation
• Horndeski stars
• The potential role of binary neutron star merger afterglows in multimessenger cosmology
• Stability of the protoneutron stars toward black hole formation
• Distinguishing modified gravity with just two tensorial degrees of freedom from general relativity: Black holes, cosmology, and matter coupling
• Gravitational Wave Sourced by Decay of Massive Particle from Primordial Black Hole evaporation
• Elliptica: a new pseudo-spectral code for the construction of initial data
• Birth and Evolution of Fast Radio Bursts: Strong Population-Based Evidence for a Neutron-Star Origin
• Forward Modelling the O3(a+b) GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions
• Universality in supernova gravitational waves with proto-neutron star properties
• Strong-interaction matter under extreme conditions from chiral quark models with nonlocal separable interactions
• Speed of sound in dense strong-interaction matter
• Disformal map and Petrov classification in modified gravity
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Temperature and Strong Magnetic Field Effects in Dense Matter
• Bulk Strong Matter: the Trinity
• Cosmological Probes of Structure Growth and Tests of Gravity
• The properties of prompt emission in short GRBs with extended emission observed by {\em Fermi}/GBM
• Rotating Love: The dynamical tides of spinning Newtonian stars
• The Legacy of Einstein's Eclipse, Gravitational Lensing
• Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity
• Gauss-Bonnet Dark Energy and the Speed of Gravitational Waves
• Prototype Superfluid Gravitational Wave Detector
• Constraining first-order phase transition inside neutron stars with application of Bayesian techniques on PSR J0437-4715 NICER data
• Modeling Gamma-ray burst Afterglow observations with an Off-axis Jet emission
• Pressure and speed of sound in two-flavor color-superconducting quark matter at next-to-leading order
• Linking Extragalactic Transients and their Host Galaxy Properties: Transient Sample, Multi-Wavelength Host Identification, and Database Construction
• A Monte-Carlo based relativistic radiation hydrodynamics code with a higher-order scheme
• Surrogate light curve models for kilonovae with comprehensive wind ejecta outflows and parameter estimation for AT2017gfo
• Generating ultra compact boson stars with modified scalar potentials
• An arm length stabilization system for KAGRA and future gravitational-wave detectors
• New covariant density functionals of nuclear matter for compact star simulations
• Radio Loud vs. Radio Quiet Gamma-ray Bursts: the Role of Binary Progenitors
• Identification of Absorption Lines of Heavy Metals in the Wavelength Range 0.97--1.32 Micron
• Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• A Bayesian study of quark models in view of recent astrophysical constraints
• Fallback Accretion Halted by R-process Heating in Neutron Star Mergers and Gamma-Ray Bursts
• On-axis scattering of scalar fields by charged rotating black holes
• Testing the nature of gravitational wave propagation using dark sirens and galaxy catalogues
• Constraints on $f(R)$ and nDGP Modified Gravity Model Parameters with Cluster Abundances and Galaxy Clustering
• Active platform stabilisation with a 6D seismometer
• Quadratic Rastall Gravity: from low-mass HESS J1731-347 to high-mass PSR J0952-0607 pulsars
• A scalable elliptic solver with task-based parallelism for the SpECTRE numerical relativity code
• Third order post-Newtonian gravitational radiation from two-body scattering: Instantaneous energy and angular momentum radiation
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• New dynamical tide constraints from current and future gravitational wave detections of inspiralling neutron stars
• The two-body potential of Vainshtein screened theories
• The Palomar Transient Factory Sky2Night programme
• Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
• KilonovaNet: Surrogate Models of Kilonova Spectra with Conditional Variational Autoencoders
• Nucleosynthesis in outflows of compact objects and detection prospects of associated kilonovae
• Rotating black holes experience dynamical tides
• Astrometric Gravitational-Wave Detection via Stellar Interferometry
• Detectability of continuous gravitational waves from isolated neutron stars in the Milky Way: the population synthesis approach
• The mirage of luminal modified gravitational-wave propagation
• Dynamical stability of the modified Tolman VII solution
• Dynamical friction from self-interacting dark matter
• Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter
• Fundamental oscillation modes of scalar bosonic dark stars
• Gravitational radiation close to a black hole horizon: Waveform regularization and the out-going echo
• Spritz: General Relativistic Magnetohydrodynamics with Neutrinos
• Lagrangian theory of structure formation in relativistic cosmology. IV. Lagrangian approach to gravitational waves
• Scalar induced gravitational waves from Chern-Simons gravity during inflation era
• Does the speed of gravitational waves depend on the source velocity?
• Are slowly rotating Ellis-Bronnikov wormholes stable?
• $f$-mode Imprints in Gravitational Waves from Coalescing Binaries involving Aligned Spinning Neutron Stars
• Towards the emergence of non-zero thermodynamical quantities for Lanczos-Lovelock black holes dressed with a scalar field
• "Stairway to Heaven" -- Spectroscopy of Particle Couplings with Gravitational Waves
• Energy extraction from rotating regular black hole via Comisso-Asenjo mechanism
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Properties of quark matter and hybrid stars from a quasiparticle model
• Revisiting Tests of Lorentz Invariance with Gamma-ray Bursts: Effects of Intrinsic Lags
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• Phantom RN-AdS black holes in noncommutative space
• The interplay of astrophysics and nuclear physics in determining the properties of neutron stars
• Forecasts on interacting dark energy with standard sirens
• Combining gravitational lensing and gravitational redshift to measure the anisotropic stress with future galaxy surveys
• Quasi-Local Black Hole Horizons: Recent Advances
• The impact of r-process heating on the dynamics of neutron star merger accretion disc winds and their electromagnetic radiation
• Incorporating the weak mixing angle dependence to reconcile the neutron skin measurement on 208Pb by PREX-II
• Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
• A Deep Targeted Search for Fast Radio Bursts from the Sites of Low-Redshift Short Gamma-Ray Bursts
• Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements
• Axisymmetric equilibrium models for magnetised neutron stars in Scalar-Tensor Theories
• Performance-Portable Binary Neutron Star Mergers with AthenaK
• Mass Distribution and Maximum Mass of Neutron Stars: Effects of Orbital Inclination Angle
• The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
• Effects of orbital precession on hyperbolic encounters
• The birth mass function of neutron stars
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• DECi-hertz Interferometer Gravitational-wave Observatory: Forecast constraints on the cosmic curvature with LSST strong lenses
• The H.E.S.S. transients follow-up system
• Entropy-limited higher-order central scheme for neutron star merger simulations
• Holographic cold dense matter constrained by neutron stars
• Implications of supermassive neutron stars for the form of the equation of state of hybrid stars
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• The FAST Galactic Plane Pulsar Snapshot Survey -- V. PSR J1901+0658 in a double neutron star system
• Relativistic stars in a cubic Galileon Universe
• Strange magnetars admixed with fermionic dark matter
• Properties of Hybrid Stars with Density Dependent Bag Model
• Compact Objects in Entangled Relativity
• Searching for Dark Clumps with Gravitational-Wave Detectors
• Fixing the dynamical evolution of self-interacting vector fields
• Tidal Love numbers of neutron stars in Rastall gravity
• Equation of state of nuclear matter and neutron stars: Quark mean-field model versus relativistic mean-field model
• Harvesting BAT-GUANO with NITRATES (Non-Imaging Transient Reconstruction And TEmporal Search): Detecting and localizing the faintest GRBs with a likelihood framework
• On the Inverse Spectrum Problem of Neutron Stars
• CMB constraints on DHOST theories
• Universal behavior of compact star based upon gravitational binding energy
• A stochastic search for intermittent gravitational-wave backgrounds
• Multi-messenger Gravitational Lensing
• Properties of binary components and remnant in GW170817 using equations of state in finite temperature field theory models
• Exploring Supernova Gravitational Waves with Machine Learning
• Constraining the equation of state in neutron-star cores via the long-ringdown signal
• Conformal Teleparallel Theories and Weyl Geometry
• Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
• Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions
• Chiral Gravitational Waves in Palatini Chern-Simons
• Probing fundamental physics with Extreme Mass Ratio Inspirals: a full Bayesian inference for scalar charge
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• Medium Effects in MIT Bag Model for quark matter: Self consistent thermodynamical treatment
• Opportunities and limits of lunar gravitational-wave detection
• Swift sky localization of gravitational waves using deep learning seeded importance sampling
• Past-directed scalar field gradients and scalar-tensor thermodynamics
• The impact of dark matter on tidal signatures in neutron star mergers with Einstein Telescope
• Scalar radiation from a source rotating around a regular black hole
• Measuring deviations from the Kerr geometry with black hole ringdown
• Fast marginalization algorithm for optimizing gravitational wave detection, parameter estimation and sky localization
• Testing gravity with gravitational wave friction and gravitational slip
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• The origin of very-high-energy gamma-rays from GRB 221009A: implications for reverse shock proton synchrotron emission
• Reverse phase transitions in binary neutron-star systems with exotic-matter cores
• Gravitational-wave constraints on scalar-tensor gravity from a neutron star and black-hole binary GW200115
• Search for Dormant Black Holes in Ellipsoidal Variables III. The OGLE BULGE Short-Period Sample
• Tidal Deformability of Neutron Stars in Scalar-Tensor Theories of Gravity
• Search for eccentric NSBH and BNS mergers in the third observing run of Advanced LIGO and Virgo
• Lower-mass-gap Black Holes in Dense Star Clusters
• Detectability of "Merger-nova" emission from a long-lived magnetar in short gamma-ray bursts
• A new automated tool for the spectral classification of OB stars
• I-Love-$⟨c_s^2⟩$: Approximately universal relations for the average neutron star stiffness
• Neutron star g-modes in the relativistic Cowling approximation
• Observing the Ping-pong Modality of Isospin Degree of Freedom in Cluster Emission from Heavy Ion Reactions
• Prospects of constraining $f(T)$ gravity with the third-generation gravitational-wave detectors
• The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Vibration isolation system with a compact damping system for power recycling mirrors of KAGRA
• The GECAM Ground Search System for Gamma-ray Transients
• Topology change, emergent symmetries and compact star matter
• Possible binary neutron star merger history of the primary of GW230529
• Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
• Spacetime-curvature induced uncertainty principle: linking the large-structure global effects to the local black hole physics
• Radial oscillations in neutron stars from QCD
• Discovering new forces with gravitational waves from supermassive black holes
• A search for supernova-like optical counterparts to ASKAP-localised Fast Radio Bursts
• Search for gravitational waves emitted from SN 2023ixf
• Bayesian Inference of dense matter equation of state of neutron star with antikaon condensation
• Binding two and three $\alpha$ particles in cold neutron matter
• Variation of delta baryon mass and hybrid star properties in static and rotating conditions
• The relative contribution to heavy metals production from binary neutron star mergers and neutron star-black hole mergers
• Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity
• Enhancing phase sensitivity in Mach-Zehnder interferometer with various detection schemes using SU(1,1) coherent states
• Braneworld Black Bounce to Transversable Wormhole
• Scalar induced gravitational waves in metric teleparallel gravity with the Nieh-Yan term
• Scalarization of isolated black holes in scalar Gauss-Bonnet theory in the fixing-the-equations approach
• A six degree-of-freedom fused silica seismometer: Design and tests of a metal prototype
• Comparison of the Characteristics of Magnetars Born in Death of Massive Stars and Merger of Compact Objects With {\em Swift} Gamma-Ray Burst Data
• Higher memory effects and the post-Newtonian calculation of their gravitational-wave signals
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
• Piezo-deformable Mirrors for Active Mode Matching in Advanced LIGO
• A new criterion for the existence of dark matter in neutron stars
• Unveiling Phase Space Modifications: A Clash of Modified Gravity and the Generalized Uncertainty Principle
• Hierarchical approach to matched filtering using a reduced basis
• Impact of biaxial birefringence in polar ice at radio frequencies on signal polarizations in ultra-high energy neutrino detection
• A hybrid approach to long-term binary neutron-star simulations
• Multi-component DHOST analysis in galaxy clusters
• Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• Radio Afterglows from Compact Binary Coalescences: Prospects for Next-Generation Telescopes
• Evolution of bare quark stars in full general relativity: Single star case
• Quintessence in the Weyl-Gauss-Bonnet model
• Simulating neutron star mergers with the Lagrangian Numerical Relativity code SPHINCS_BSSN
• The Equation of State of Neutron-Rich Matter at Fourth Order of Chiral Effective Field Theory and the Radius of a Medium-Mass Neutron Star
• Quark-hadron pasta phase in neutron stars: the role of medium-dependent surface and curvature tensions
• Scalar Hairy Black Holes with Inverted Mexican Hat Potential
• On the detection of the electromagnetic counterparts from lensed gravitational wave events by binary neutron star mergers
• Hybrid Stars Built with Density Dependent Models
• Radial and Non-Radial Oscillations of Inverted Hybrid Stars
• Massive relativistic compact stars from SU(3) symmetric quark models
• Gravitational wave memory of compact binary coalescence in the presence of matter effects
• A Comprehensive Analysis of the Gravitational Wave Events with the Hilbert-Huang Transform: From Compact Binary Coalescence to Supernova
• Rescaling strange-cluster stars and its implications on gravitational-wave echoes
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Dark Stars and Gravitational Waves: Topical Review
• Hybrid stars with reactive interfaces: analysis within the Nambu-Jona-Lasinio model
• Understanding the progenitor formation galaxies of merging binary black holes
• Signatures of quark deconfinement through the r-modes of twin stars
• Bayesian model selection for GRB 211211A through multi-wavelength analyses
• Neutron Stars in Modified Teleparallel Gravity
• Target of Opportunity Observations Detectability of Kilonovae with WFST
• Debiasing Standard Siren Inference of the Hubble Constant with Marginal Neural Ratio Estimation
• Light Axiodilatons: Matter Couplings, Weak-Scale Completions and Long-Distance Tests of Gravity
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Radioactively-Powered Gamma-Ray Transient Associated with a Kilonova from Neutron Star Merger
• Enabling the discovery of fast transients: A kilonova science module for the Fink broker
• A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
• The effects of Time-Variable Absorption due to Gamma-Ray Bursts In Active Galactic Nuclei Accretion Disks
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• AT2018lqh and the nature of the emerging population of day-scale duration optical transients
• Baryonic dense matter in view of gravitational-wave observations
• Reviving Horndeski after GW170817 by Kaluza-Klein compactifications
• Quasi-universal relations for generalized Skyrme stars
• SLICK: Strong Lensing Identification of Candidates Kindred in gravitational wave data
• Towards observing the neutron star collapse with gravitational wave detectors
• Exploring field-evolution and dynamical-capture coalescing binary black holes in GWTC-3
• High-precision nuclear chronometer for the cosmos
• Tidal Deformability of Strange Quark Planets and Strange Dwarfs
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves
• Role of the symmetry energy slope in neutron stars: exploring the model-dependency
• Systematic errors due to quasi-universal relations in binary neutron stars and their correction for unbiased model selection
• Neutron matter from local chiral effective field theory interactions at large cutoffs
• Combined X-ray and optical analysis to probe the origin of the plateau emission in $\gamma$-ray bursts afterglows
• Geometric and thermodynamic characterization of binary neutron star accretion discs
• Full analytic expression of overlap reduction function for gravitational wave background with pulsar timing arrays
• Measuring neutron-star distances and properties with gravitational-wave parallax
• Observational constraints on the origin of the elements. VI. Origin and evolution of neutron-capture elements as probed by the Gaia-ESO survey
• Gravitational waves from neutron-star mountains
• Observing the dark sector
• Nonparametric Representation of Neutron Star Equation of State Using Variational Autoencoder
• Constraining the ellipticity of new-born magnetar with the observational data of Long gamma-ray bursts
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• Experimental study of the isospin transport with 40,48 Ca+ 40,48 Ca reactions at 35 MeV/nucleon
• Tidal Deformability Doppelgangers: Implications of a low-density phase transition in the neutron star equation of state
• Polarized gravitational waves in the parity violating scalar-nonmetricity theory
• Gravitational radiation in higher order non-local gravity
• Irregular universe in the Nieh-Yan modified teleparallel gravity
• Empirical neutron star mass formula based on experimental observables
• Optical follow-up observation for GW event S190510g using Subaru/Hyper Suprime-Cam
• Probing the primordial Universe with 21-cm line from cosmic dawn/epoch of reionization
• Time evolution of the local gravitational parameters and gravitational wave polarizations in a relativistic MOND theory
• Detection possibility of continuous gravitational waves from rotating magnetized neutron stars
• Planetary seismology as a test of modified gravity proposals
• A proposed deep sea Neutrino Observatory in the Nanhai
• Gravitationally Lensed Orphan Afterglows of Gamma-Ray Bursts
• Giant planet formation in Palatini gravity
• Gravitational Waves in the Presence of Viscosity
• Quasinormal modes and echo effect of cylindrical anti-de Sitter black hole spacetime with a thin shell
• Imprints of the nuclear symmetry energy slope in gravitational wave signals emanating from neutron stars
• Observational limits on the rate of radiation-driven binary black hole capture events
• Polarization modes of gravitational waves in generalized Proca theory
• Estimating magnetar radii with an empirical meta-model
• Probing the Fermi-LAT GeV excess with gravitational waves
• Numerical Inside View of Hypermassive Remnant Models for GW170817
• Relativistic correction to the r-mode frequency in light of multi-messenger constraints
• Assessment of a new sub-grid model for magneto-hydrodynamical turbulence. I. Magnetorotational instability
• Constraining modified gravity theories with scalar fields using black-hole images
• A minimal self tuning model to solve the cosmological constant problem
• Hybrid stars with large quark cores within the parity doublet model and modified NJL model
• Shear and interface modes in neutron stars with pasta structures
• Blandford-Znajek jets in MOdified Gravity
• LION :Laser Interferometer On the mooN
• Multipole tidal effects in the post-Newtonian gravitational-wave phase of compact binary coalescences
• Quadratic DHOST theories revisited
• Many-body approximations to the superfluid gap and critical temperature in pure neutron matter
• Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO
• Black hole hyperaccretion in collapsars. II. Gravitational waves
• Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis
• GWSkyNet-Multi: A Machine Learning Multi-Class Classifier for LIGO-Virgo Public Alerts
• Astrophysics with heavy-ion beams
• Constraint on hybrid stars with gravitational wave events
• Novel regular black holes: geometry, source and shadow
• Effects of nuclear matter properties in neutron star mergers
• Prompt sky localization of compact binary sources using a meshfree approximation
• Testing cosmic opacity with the combination of strongly lensed and unlensed supernova Ia
• On spin optics for gravitational waves lensed by a rotating object
• Probing resonant excitations in exotic compact objects via gravitational waves
• Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology
• Emergence of new oscillation modes in dark matter admixed neutron stars
• How can LISA probe a population of GW190425-like binary neutron stars in the Milky Way?
• Assessing equation of state-independent relations for neutron stars with nonparametric models
• Self-gravitating magnetised tori around black holes in general relativity
• Distinguishing black holes with and without spontaneous scalarization in Einstein-scalar-Gauss-Bonnet theories via optical features
• Dark matter relic density from conformally or disformally coupled light scalars
• Maximum Mass Of Differentially Rotating Strange Quark Stars
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• GECKO Optical Follow-up Observation of Three Binary Black Hole Merger Events: GW190408_181802, GW190412, and GW190503_185404
• The orbital-decay test of general relativity to the 2% level with 6-year VLBA astrometry of the double neutron star PSR J1537+1155
• Coherence scale of magnetic fields generated in early-time forward shocks of GRBs
• Universal relations for anisotropic interacting quark stars
• Measuring the primordial gravitational wave background in the presence of other stochastic signals
• Gravitational Wave Displacement and Velocity Memory Effects
• Damping of density oscillations from bulk viscosity in quark matter
• Rotating Kerr-Newman space-times in Metric-Affine Gravity
• Using gravitational waves to distinguish between neutron stars and black holes in compact binary mergers
• Constraining the AGN formation channel for detected black hole binary mergers up to z=1.5 with the Quaia catalogue
• Impact of nuclear matter properties on the nucleosynthesis and the kilonova from binary neutron star merger ejecta
• Kinematic constraints on the ages and kick velocities of Galactic neutron star binaries
• Quasinormal modes of slowly-spinning horizonless compact objects
• Long-duration transient, gravitational-wave search pipeline
• Dark matter admixed neutron stars with a realistic nuclear equation of state from chiral nuclear interactions
• Sensitivity of third-generation interferometers to extra polarizations in the Stochastic Gravitational Wave Background
• Comparing the luminosity distance for gravitational waves and electromagnetic signals in a simple model of quadratic gravity
• thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state
• Magnetic deformation of neutron stars in scalar-tensor theories
• Gravitational waves in higher-order $R^2$ gravity
• Emulators for scarce and noisy data: application to auxiliary field diffusion Monte Carlo for the deuteron
• From finite nuclei to neutron stars : the essential role of high-order density dependence in effective forces
• Strongly Magnetized Hot QCD Matter and Stochastic Gravitational Wave Background
• Searching for Axion-Like Particles from Core-Collapse Supernovae with Fermi LAT's Low Energy Technique
• Shear oscillations in neutron stars and the nuclear symmetry energy
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
• Constraining Properties of GRB Central Engines with X-ray flares
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• No slip gravity in light of LISA standard sirens
• Non-homogeneous exoplanets in metric-affine gravity
• Isolated pulsar population synthesis with simulation-based inference
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• Effects of Onset of Phase Transition on Binary Neutron Star Mergers
• Collective plasma effects of electron-positron pairs in beam-driven QED cascades
• The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars
• Probing modified gravitational-wave propagation through tidal measurements of binary neutron star mergers
• Enhancing interferometer sensitivity without sacrificing bandwidth and stability: beyond single-mode and resolved-sideband approximation
• Binary systems in massive scalar-tensor theories: Next-to-leading order gravitational wave phase from effective field theory
• Isotropic and anisotropic neutron star structure in 4D Einstein Gauss Bonnet Gravity
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Tidal-heating/viscous dissipation correspondence in black holes and viscous compact objects
• Quark-quark interaction and quark matter in neutron stars
• The implications of stochastic gas torques for asymmetric binaries in the LISA band
• Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term
• Fuzzy Dark Matter in Relativistic Stars
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• An exact model of a gravitational wave in the Bianchi III universe based on Shapovalov II wave spacetime and the quadratic theory of gravity
• Polytropic fits of modern and unified equations of state
• Quantifying effects of inhomogeneities and curvature on gravitational wave standard siren measurements of $H(z)$
• GROWTH on S190426c II: GROWTH-India Telescope search for an optical counterpart with a custom image reduction and candidate vetting pipeline
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• Direct mapping of tidal deformability to the iso-scalar and iso-vector nuclear matter parameters
• Neutrino Flavor Transformation in Neutron Star Mergers
• Boosting the sensitivity of high frequency gravitational wave detectors by PT-symmetry
• Reconstruction of the neutron star equation of state from $w$-quasinormal modes spectra with a piecewise polytropic meshing and refinement method
• Cosmological determination to the values of the prefactors in the logarithmic corrected entropy-area relation
• Differentially rotating scalarized neutron stars with realistic post-merger profile
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
• The luminosity functions of kilonovae from binary neutron star mergers under different equation of states
• Modeling the GRB jet properties with 3D general relativistic simulations of magnetically arrested accretion flows
• Precision Ephemerides for Gravitational-wave Searches -- IV: Corrected and refined ephemeris for Scorpius X-1
• Long-Lived Quasinormal Modes of Brane-Localized Reissner-Nordström--de Sitter Black Holes
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
• Photometric and Spectroscopic Observations of GRB 190106A: Emission from Reverse and Forward Shocks with Late-time Energy Injection
• Calibration of the Advanced Spectral Leakage scheme for neutron star merger simulations, and extension to smoothed-particle hydrodynamics
• Efficient fully precessing gravitational waveforms for binaries with neutron stars
• Thermodynamics of static and stationary black holes in Einstein-Gauss-Bonnet gravity with dark matter
• Detecting dense-matter phase transition signatures in neutron star mass-radius measurements as data anomalies using normalising flows
• Dispersion of Light Traveling through the Interstellar Space, Induced and Intrinsic Lorentz Invariance Violation
• Detectability of Sub-Solar Mass Neutron Stars Through a Template Bank Search
• How does dark matter affect compact star properties and high density constraints of strongly interacting matter
• Gravitational waves from strong first order phase transitions
• Robustness of kinetic screening against matter coupling
• Systematic study of surface properties for Ne, Na, Mg, Al and Si isotopes in a coherent density fluctuation model using the relativistic mean field formalism
• Bayesian Inverse Problem of Rotating Neutron Stars
• Population properties of neutron stars in the coalescing compact binaries
• Impact of unmodeled eccentricity on the tidal deformability measurement and implications for gravitational wave physics inference
• Stringent Tests of Gravity with Highly Relativistic Binary Pulsars in the Era of LISA and SKA
• Deflection angle with electromagnetic interaction and gravitational-electromagnetic dual lensing
• Effect of dark matter interaction on hybrid star in the light of the recent astrophysical observations
• Cosmological Tests of Gravity: A Future Perspective
• Comparative study of 1D and 2D convolutional neural network models with attribution analysis for gravitational wave detection from compact binary coalescences
• Black-Hole Neutron Star Simulations with the BAM code: First Tests and Simulations
• Testing gravity with interstellar precursor missions
• On the Role of Muons in Binary Neutron Star Mergers: First Simulations
• The sound-ring radiation of expanding vortex clusters
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• Variability in Short Gamma-ray Bursts: Gravitationally Unstable Tidal Tails
• Classification of Gravitational Waves in Higher-dimensional Space-time and Possibility of Observation
• Bouncing behavior in $f(R,L_m)$ gravity: Phantom crossing and energy conditions
• GRB 170817A Afterglow from a Relativistic Electron-Positron Pair Wind Observed Off-axis
• Premerger phenomena in neutron-star binary coalescences
• Analysis of the subsolar-mass black hole candidate SSM200308 from the second part of the third observing run of Advanced LIGO-Virgo
• Multi-messenger astronomy with INTEGRAL
• Gravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Polarization modes of gravitational waves in general modified gravity: General metric theory and general scalar-tensor theory
• Revisiting the post-glitch relaxation of the 2000 Vela glitch with the neutron star equation of states in the Brueckner and relativistic Brueckner theories
• f-mode oscillations of anisotropic neutron stars in full general relativity
• Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds
• Gravitational Waves from Phase Transitions
• Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
• Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model
• Line Expansion Opacity in Relativistically Expanding Media
• Universality in quasinormal modes of neutron stars with quark-hadron crossover
• r-Process Nucleosynthesis and Radioactively Powered Transients from Magnetar Giant Flares
• Bulk viscosity of two-color superconducting quark matter in neutron star mergers
• Compact binary systems in Einstein-Aether gravity: Direct integration of the relaxed field equations to 2.5 post-Newtonian order
• Deviation of geodesics and particle trajectories in a gravitational wave of the Bianchi type VI universe
• Neural network time-series classifiers for gravitational-wave searches in single-detector periods
• Mitigating the binary viewing angle bias for standard sirens
• Metallicity-Suppressed Collapsars Cannot be the Dominant r-Process Source in the Milky Way
• Swarm-intelligent search for gravitational waves from eccentric binary mergers
• Identifying Spin Properties of Evaporating Black Holes through Asymmetric Neutrino and Photon Emission
• Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations
• The non-relativistic limit of first-order relativistic viscous fluids
• Continuous gravitational wave emission from neutron stars with pinned superfluids in the core
• Emulators for Scarce and Noisy Data: Application to Auxiliary-Field Diffusion Monte Carlo for Neutron Matter
• Effect of inhomogeneities on the propagation of gravitational waves from binaries of compact objects
• Extragalactic neutrino emission induced by Supermassive and Stellar Mass Black Hole mergers
• Impact of dipolar magnetic fields on gravitational wave strain by galactic binaries
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• The Signature of Refreshed Shocks in the of Afterglow of GRB030329
• Fast neutrino cooling in the accreting neutron star MXB 1659-29
• Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
• Properties of quark-matter cores in massive hybrid stars
• Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
• Weak gravity on a $\Lambda$CDM background
• Localization of gravitational waves using machine learning
• Slowly-rotating compact objects: the nonintegrability of Hartle-Thorne particle geodesics
• Dynamical Dark Energy in Minimally Modified Gravity
• Dynamics of Binary System around Supermassive Black Hole
• Third post-Newtonian gravitational radiation from two-body scattering II. Hereditary Energy radiation
• Comprehensive Analysis of Constructing Hybrid Stars with an RG-consistent NJL Model
• Swampland Criteria and Constraints on Inflation in a $f(R,T)$ Gravity Theory
• LOFAR 144-MHz follow-up observations of GW170817
• Magnetar central engines in gamma-ray busts follow the universal relation of accreting magnetic stars
• Discovery of a Universal Correlation For Long and Short GRBs and Its Application on the Study of Luminosity Function and Formation Rate
• Hamilton's equations in the covariant teleparallel equivalent of general relativity
• Revisiting Vainshtein Screening for fast N-body simulations
• Optimal Optical Search Strategy for Finding Transient in Large Sky Error Region Under Realistic Constraints
• Non-radial oscillations and gravitational wave emission of hybrid neutron stars
• New Non-Abelian Reissner-Nordström Black Hole Solutions in the Generalized SU(2) Proca Theory And Some Astrophysical Implications
• Rapid localization of gravitational wave hosts with FIGARO
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Late-time post-merger modeling of a compact binary: effects of relativity, r-process heating, and treatment of transport effects
• Boltzmann equations for astrophysical Stochastic Gravitational Wave Backgrounds scattering off of massive objects
• Dynamics of a relativistic jet through magnetized media
• Gamma-ray Diagnostics of r-process Nucleosynthesis in the Remnants of Galactic Binary Neutron-Star Mergers
• The study of nonstrange quark stars within a modified NJL model
• Cold quark matter in a quasiparticle model: thermodynamic consistency and stellar properties
• Cautionary tales on heating-rate prescriptions in kilonovae
• Generalized nonconservative gravitational field equations from Herglotz action principle
• Postmerger multimessenger analysis of binary neutron stars: Effect of the magnetic field strength and topology
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• Formation of GW230529 from Isolated Binary Evolution
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• High-Order Multipole and Binary Love Number Universal Relations
• Bayesian inference of strangeon matter using the measurements of PSR J0437-4715 and GW190814
• Dense matter equation of state and phase transitions from a Generalized Skyrme model
• Search for Coincident Gravitational-wave and Fast Radio Burst Events from 4-OGC and the First CHIME/FRB Catalog
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Gamma-Ray Burst in a Binary System
• Gravitational Waves from Newborn Accreting Millisecond Magnetars
• Early warning of precessing compact binary merger with third-generation gravitational-wave detectors
• Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations
• Tidal effects in gravitational waves from neutron stars in scalar-tensor theories of gravity
• Hyperons, deconfinement and the speed of sound in neutron stars
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities
• Case for quarkyoniclike matter from a constituent quark model
• High-energy neutrino emission associated with gravitational-wave signals: effects of cocoon photons and constraints on late-time emission
• (Anti)kaon condensation in strongly magnetized dense matter
• Primordial Clocks within Stochastic Gravitational Wave Anisotropies
• Constraining cosmological parameters from strong lensing with DECIGO and B-DECIGO sources
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Quasinormal Modes and Gray-Body Factors for Gravitational Perturbations in Asymptotically Safe Gravity
• Generalised Proca Theories in Teleparallel Gravity
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• In search of short gamma-ray burst optical counterpart with the Zwicky Transient Facility
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• GW170817: A Neutron Star Merger in a Mass-Transferring Triple System
• Angle-dependent in-situ fast flavor transformations in post-neutron star merger disks
• Low frequency electromagnetic radiation coming from gravitational waves generated by neutron stars
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Scalar Perturbation Around Rotating Regular Black Hole: Superradiance Instability and Quasinormal Modes
• Bounds on tidal charges from gravitational-wave ringdown observations
• Gravitational wave constraints on extended dark matter structures
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• Influence of the nuclear symmetry energy slope on observables of compact stars with $\Delta$-admixed hypernuclear matter
• Kinetic modeling of the electromagnetic precursor from an axisymmetric binary pulsar coalescence
• Chemical Evolution of R-process Elements in Stars (CERES). III. Chemical abundances of neutron capture elements from Ba to Eu
• Effects from Dark Matter Halos on X-ray Pulsar Pulse Profiles
• Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms
• Fundamental Relations between Measurement, Radiation and Decoherence in Gravitational Wave Laser Interferometer Detectors
• Gravitational waves and primordial black holes from chirality imbalanced QCD first-order phase transition with $\mathcal{P}$ and $\mathcal{C}\mathcal{P}$ violation
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Dark photon bursts from compact binary systems and constraints
• Burst search method based on likelihood ratio in Poisson Statistics
• Source localizations with the network of space-based gravitational wave detectors
• Disformal mappings of spherical DHOST geometries
• High-accuracy high-mass ratio simulations for binary neutron stars and their comparison to existing waveform models
• Multi-messenger Emission from Tidal Waves in Neutron Star Oceans
• Neutron Skins: Weak Elastic Scattering and Neutron Stars
• Isochronous mass spectrometry at the RIKEN Rare-RI Ring facility
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Gravitational Spectra and Wave Propagation in Regular Black Holes Supported by a Dehnen Halo
• Imprint of Early Dark Energy in Stochastic Gravitational Wave Background
• Prospects of calibrating afterglow modeling of short GRBs with gravitational wave inclination angle measurements and resolving the Hubble tension with a GW-GRB association event
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• Dark-siren Cosmology with Decihertz Gravitational-wave Detectors
• Constraining the nuclear equation of state via gravitational-wave radiation of short gamma-ray burst remnants
• The Jiao Tong University Spectroscopic Telescope Project
• Influence of neutrino-electron scattering and neutrino-pair annihilation on hypermassive neutron star
• Spontaneous Radiation of Black Holes
• Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains
• Echoes of axial gravitational perturbations in stars of uniform density
• GRB 080503: A very early blue kilonova and an adjacent non-thermal radiation component
• J-GEM optical and near-infrared follow-up of gravitational wave events during LIGO's and Virgo's third observing run
• Hybrid stars may have an inverted structure
• Signature of hadron-quark crossover in binary-neutron-star mergers
• GRB 111005A at Z = 0.0133 and the Prospect of Establishing Long-short GRB/GW Association
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• Hyperonic uncertainties in neutron stars, mergers and supernovae
• Incompressibility and Symmetry Energy of Neutron Star
• Spin-down induced quark-hadron phase transition in cold isolated neutron stars
• Search of QCD phase transition points in the canonical approach of the NJL model
• Quantum precision limits of displacement noise free interferometers
• AsterX: a new open-source GPU-accelerated GRMHD code for dynamical spacetimes
• Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Constraining Palatini gravity with GR-independent equations of state for neutron stars
• Quasi-universal relations in the context of future neutron star detections
• Reconstruction of multiple Compton scattering events in MeV gamma-ray Compton telescopes towards GRAMS: the physics-based probabilistic model
• Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis
• Horndeski fermion-boson stars
• The impact of nuclear reactions on the neutron-star g-mode spectrum
• Tidal Forces in Majumdar-Papapetrou Spacetimes
• Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
• Constraints and correlations of nuclear matter parameters from a density-dependent van der Waals model
• Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
• Gravitational Waves of Type III Shapovalov Spacetimes: Particle Trajectories, Geodesic Deviation and Tidal Accelerations
• Solar System Tests in Brans-Dicke and Palatini f(R)-theories
• Pulsar Glitch in a Strangeon Star Model. III. The recovery
• A tight universal relation between the shape eccentricity and the moment of inertia for rotating neutron stars
• Hidden symmetry between rotational tidal Love numbers of spinning neutron stars
• Towards a Precision Measurement of Binary Black Holes Formation Channels Using Gravitational Waves and Emission Lines
• Modification of the mean free path of very high energy photons due to a relativistic deformed kinematics
• Experimental study of the ${}^{40,48}$Ca+ ${}^{40,48}$Ca reactions at 35 MeV/nucleon
• Constraining exotic compact stars composed of bosonic and fermionic dark matter with gravitational wave events
• Reinvestigation of Fast Radio Burst Host Galaxy and Event Rate Density
• Gravitational wave modes in matter
• Cosmic Cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure
• Late time cosmological evolution in DHOST models
• Gravitational waves from inspiraling black holes in quadratic gravity
• Standard cooling of rapidly rotating isolated neutron stars in 2D
• Host galaxy identification for binary black hole mergers with long baseline gravitational wave detectors
• Chaotic Inflation and Reheating in Generalized Scalar-Tensor Gravity
• New evidence of multiple channels for the origin of gamma-ray bursts with extended emission
• Long-lived quasinormal modes, shadows and particle motion in four-dimensional quasi-topological gravity
• Kerr-Enhanced Optical Spring
• $2\cdot 10^{-13}$ fractional laser frequency stability with a 7-cm unequal-arm Mach-Zehnder interferometer
• Linear and Second-order Geometry Perturbations on Spacetimes with Torsion
• Study on the detectability of gravitational radiation from single-binary encounters between black holes in nuclear star cluster: the case of hyperbolic flybys
• Fully general relativistic simulations of rapidly rotating quark stars: Oscillation modes and universal relations
• Probing Spin-Induced Quadrupole Moments in Precessing Compact Binaries
• Constraining the relativistic mean-field models from PREX-2 data: Effective forces revisited
• Revealing Phase Transition in Dense Matter with Gravitational Wave Spectroscopy of Binary Neutron Star Mergers
• Impact of jets on kilonova photometric and polarimetric emission from binary neutron star mergers
• Thermal effects in hot and dilute homogeneous asymmetric nuclear matter
• Probing particle acceleration at trans-relativistic shocks with off-axis gamma-ray burst afterglows
• Numerically modeling Brownian thermal noise in amorphous and crystalline thin coatings
• Slowly Rotating Neutron Star with Holographic Multiquark Core: I-Love-Q Relations
• Magnetic dissipation in short gamma-ray burst jets. I. Resistive relativistic MHD evolution in a model environment
• Implementing a new recovery scheme for primitive variables in the general relativistic magnetohydrodynamic code Spritz
• Spherically symmetric anisotropic strange stars
• Hair-dressing Horndeski: an approach to hairy solutions in cubic Horndeski gravity
• Reconstruction method in the kinetic gravity braiding theory with shift-symmetric
• Prospects of Gravitational Wave Follow-up Through a Wide-field Ultra-violet Satellite: a Dorado Case Study
• Detection of gravitational wave mixed polarization with single space-based detectors
• Impact of level densities and $\gamma$-strength functions on $r$-process simulations
• Response of the first POLAR-2 Prototype to Polarized Beams
• Europium enrichment and hierarchical formation of the Galactic halo
• CALET Search for electromagnetic counterparts of gravitational waves during the LIGO/Virgo O3 run
• A convolutional neural network to distinguish glitches from minute-long gravitational wave transients
• Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
• Quantum coherence of relic gravitons and Hanbury Brown-Twiss interferometry
• Classical Love for Quantum Blackholes
• Testing the Paradigm of Nuclear Many-Body Theory
• Estimation of the gravitational wave polarizations from a non template search
• Spontaneous scalarization of charged stars
• Stability of hypermassive neutron stars with realistic rotation and entropy profiles
• Quasibound state reminiscent in de-Sitter black holes: Quasinormal modes and the decay of massive fields
• A new look at the Bondi-Sachs energy-momentum
• Vainshtein screening for slowly rotating stars
• Compact stars in the Einstein dark energy model
• Multimessenger Universe with Gravitational Waves from Binaries
• Global high-order numerical schemes for the time evolution of the general relativistic radiation magneto-hydrodynamics equations
• Self-tuning kinetic gravity braiding: Cosmological dynamics, shift symmetry, and the tadpole
• Improving cosmological reach of a gravitational wave observatory using Deep Loop Shaping
• Chaos in Inhomogeneous Neutrino Fast Flavor Instability
• Gravitational Radiation from Eccentric Binary Black Hole System in Dynamical Chern-Simons Gravity
• Prospects of Probing Dark Matter Condensates with Gravitational Waves
• Core structures of vortices in Ginzburg-Landau theory for neutron ${}^3{P}_2$ superfluids
• Possibility of a coordinated signaling scheme in the Galaxy and SETI experiments
• Astrophysical reaction rates with realistic nuclear level densities
• On the formation of "supermassive" neutron stars and dynamical transition to spontaneous scalarization
• Scalar emission from neutron star-black hole binaries in scalar-tensor theories with kinetic screening
• Gravitational influence of high power laser pulses
• Test the Weak Cosmic Supervision Conjecture in Dark Matter-Black Hole System
• Probing the impact of Delta-Baryons on Nuclear Matter and Non-Radial Oscillations in Neutron Stars
• Inference of multi-channel r-process element enrichment in the Milky Way using binary neutron star merger observations
• Femtoscopic study of the $\Lambda \alpha$ interaction
• Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity
• Quasinormal modes of scalar field coupled to Einstein's tensor in the non-commutative geometry inspired black hole
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Effects of mirror birefringence and its fluctuations to laser interferometric gravitational wave detectors
• Tidal Deformation and Radial Pulsations of Neutron Star with Holographic Multiquark Core
• Constraints on Equivalence Principle Violation from Gamma Ray Bursts
• Motion of test particle in rotating boson star
• Multiplexing lobster-eye optics: a concept for wide-field X-ray monitoring
• Thermodynamic Consistent Description of Compact Stars of Two Interacting Fluids: The Case of Neutron Stars with Higgs Portal Dark Matter
• Continuous gravitational waves from trapped magnetar ejecta and the connection to glitches and antiglitches
• Fundamental physics with neutron stars
• A new first-order formulation of the Einstein equations exploiting analogies with electrodynamics
• 21 cm power spectrum in interacting cubic Galileon model
• Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
• Shift-symmetric Horndeski gravity in the asymptotic-safety paradigm
• Kerr Black Hole in Einstein--Æther Gravity
• Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
• Kaon condensation in skyrmion matter and compact stars
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Aether scalar tensor theory: Hamiltonian Formalism
• Inferring the Equation of State from Neutron Star Observables via Machine Learning
• Competition between allowed and first-forbidden $\beta$ decay in $r$-process waiting-point nuclei within a relativistic beyond-mean-field approach
• Astrophysical insights into magnetic Penrose process around parameterized Konoplya-Rezzolla-Zhidenko black hole
• Problematic systematics in neutron-star merger simulations
• Black Hole singularity and its possible mitigations: Reformulation of Penrose Singularity theorem using null Raychaudhuri matrix
• Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Black hole-neutron star mergers with massive neutron stars in numerical relativity
• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
• Quantum Squeezing Schemes for Heterodyne Readout
• Proposed Lunar Measurements of $r$-Process Radioisotopes to Distinguish Origin of Deep-sea 244Pu
• Multi-spectral Sirens: Gravitational-wave Cosmology with (Multi-) Sub-populations of Binary Black Holes
• Analyzing the dense matter equation of states in the light of the compact object HESS J1731-347
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Massive neutron stars as mass gap candidates: Exploring equation of state and magnetic field
• Neutron Stars In $f(R,T)$ Theory: Slow Rotation Approximation
• Prospects for the inference of inertial modes from hypermassive neutron stars with future gravitational-wave detectors
• Searching for wormholes with gravitational wave scattering
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Whispers from the quantum core: the ringdown of semiclassical stars
• The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers
• Inflation driven by massive vector fields with derivative self-interactions
• Black Holes merging with Low Mass Gap Objects inside Globular Clusters
• Generalized McVittie geometry in Horndeski gravity with matter
• A Markov Chain Monte Carlo approach for measurement of jet precession in radio-loud active galactic nuclei
• Horndeski Proca stars with vector hair
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• Element formation in radiation-hydrodynamics simulations of kilonovae
• Building post-Newtonian neutron stars
• Dark energy with a shift-symmetric scalar field: obstacles, loophole hunting and dead ends
• Action-angle variables of a binary black hole with arbitrary eccentricity, spins, and masses at 1.5 post-Newtonian order
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• On the Testability of the Quark-Hadron Transition Using Gravitational Waves From Merging Binary Neutron Stars
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• K2: Background Survey -- the search for undiscovered transients in Kepler/K2 data
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• Neutron Stars in Palatini $R+\alpha R^2$ and $R+\alpha R^2+\beta Q$ Theories
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• On the nature of compact stars determined by gravitational waves, radio-astronomy, x-ray emission and nuclear physics
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• Astrophysics in Strong Electromagnetic Fields and Laboratory Astrophysics
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• Generalized Horndeski-Like Einstein Gauss-Bonnet Inflation with Massless Primordial Gravitons
• The AGILE real-time analysis pipelines in the multi-messenger era
• Maximum mass of hybrid star formed via shock induced phase transition in cold neutron stars
• Probing Particle Physics with Gravitational Waves
• r-mode instability of neutron stars in low-mass X-ray binaries: effects of Fermi surface depletion and superfluidity of dense matter
• Mid-Frequency Gravitational Wave Detection and Sources
• Detectability of radio afterglows from binary neutron star mergers and implications for fast radio bursts
• Neutron star equation of state and tidal deformability with nuclear energy density functionals
• The Luminosity Distribution of Short Gamma-Ray Bursts under a Structured Jet Scenario
• Role of $\Delta$s in determining the properties of Neutron Stars in parameterized hydrostatic equilibrium
• Can we constrain the aftermath of binary neutron star mergers with short gamma-ray bursts?
• Multipole analysis on gyroscopic precession in $f(R)$ gravity with irreducible Cartesian tensors
• The remnant of neutron star-white dwarf merger and the repeating fast radio bursts
• Discrete and Continuous Ejection Models of the Radio Source Associated with GW170817
• The Advanced X-ray Imaging Satellite
• The effective field theory of dark energy diagnostic of linear Horndeski theories after GW170817 and GRB170817A
• Astro2020 Science White Paper: Radio Counterparts of Compact Object Mergers in the Era of Gravitational-Wave Astronomy
• Black Hole - Neutron Star Binary Mergers: The Imprint of Tidal Deformations and Debris
• Astrophysical neutrinos: theory
• 2D End-to-End Modeling of Kilonovae from Binary Neutron Star Merger Remnants
• IIb or not IIb: A Catalog of ZTF Kilonova Imposters
• Speed of sound peak in isospin QCD: a natural prediction of the Medium Separation Scheme
• Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
• Axion effects on quark matter and quark-matter cores in massive hybrid stars
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• WINTER on S250206dm: A near-infrared search for an electromagnetic counterpart to a gravitational-wave event
• Interferometer Euro-Asian Network: Detection Characteristics for Signals of Known Shape
• Improving force sensitivity by amplitude measurement of light reflected from a detuned optomechanical cavity
• Tidal deformability of neutron stars with exotic particles within a density dependent relativistic mean field model in R-squared gravity
• $M/R$ estimates for two neutron stars in LMXBs with possible r-mode frequencies detected
• A General Overview for Localizing Short Gamma-ray Bursts with a CubeSat Mega-Constellation
• Chiral asteroseismology: seismic oscillations caused by chiral transport in neutron stars and supernovae
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• Optimized localization for gravitational-waves from merging binaries
• $g$-mode oscillations of dark matter admixed neutron stars
• The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
• Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
• Some cosmological features of 4D Gauss-Bonnet gravity with varying cosmological constant
• Constraining the effective field theory of dark energy with multimessenger astronomy
• How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
• The sounds of science a symphony for many instruments and voices part II
• Interpolated kilonova spectra models: necessity for a phenomenological, blue component in the fitting of AT2017gfo spectra
• Challenges to a sharp change in $G$ as a solution to the Hubble tension
• Tidal deformation of black holes in Lovelock gravity
• The mass, spin and rotational energy of the remnant black holes from compact binary mergers
• Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
• Slow-roll approximations in Einstein--Gauss--Bonnet gravity formulated in terms of e-folding numbers
• New measures to test modified gravity cosmologies
• Gravitational collapse in Quadratic Gravity
• Dark Matter phenomenology : from simplified WIMP models to refined alternative solutions
• Evolving wormhole formation in dRGT massive gravity
• Dark matter effects in modified teleparallel gravity
• GRB Afterglow of the Sub-relativistic Materials with Energy Injection
• Gravitational wave asteroseismology of accreting neutron stars in a steady state
• Lanczos equation on light-like hypersurfaces in a cosmologically viable class of kinetic gravity braiding theories
• Comparison of neural network architectures for feature extraction from binary black hole merger waveforms
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• Large black-hole scalar charges induced by cosmology in Horndeski theories
• Data-driven approach for modeling the temporal and spectral evolution of kilonova systematic uncertainties
• Necessity of selfconsistent calculations for the electromagnetic field in probing the nuclear symmetry energy using pion observables in heavy-ion collisions
• X-raying the Birth of Binary Neutron Stars and Neutron Star-Black Hole Binaries
• A protocol of potential advantage in the low frequency range to gravitational wave detection with space based optical atomic clocks
• Neutron stars in general relativity and scalar-tensor theory of gravity
• Dependence of postmerger properties on the thermal heating efficiency in neutron star mergers
• Energy conditions in a modified Brans-Dicke theory
• Does fractal Universe favour warm inflation: Observational support?
• Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
• Distinguishing compact objects in extreme-mass-ratio inspirals by gravitational waves
• Revisit to the yield ratio of triton and ${}^3$He as an indicator of neutron-rich neck emission
• The RTApipe framework for the gamma-ray real-time analysis software development
• Probing eccentric higher-order modes through an effective chirp mass model
• Strong Lensing Effect and Quasinormal Modes of Oscillations of Black Holes in $\mathbf{f}(\mathbf{R},\mathbf{T})$ Gravity Theory
• Impact of dark matter on strange quark stars described by different quark models
• Optical ultra-stable optical clock cavities as resonant mass gravitational wave detectors in search for new physics
• New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations
• Impact of $\Xi$-Hypernuclear Constraints on Relativistic Equation of State and Properties of Hyperon Stars
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• Second-order corrections to Starobinsky inflation
• Quark deconfinement in compact stars through sexaquark condensation
• $S$-matrix approach to general gravity and beyond
• Extended search for supernova-like neutrinos in NOvA coincident with LIGO/Virgo detections
• Gravitational Wave Signatures of Primordial Black Hole Reheating in Upcoming Interferometry Missions
• Gravitational wave energy momentum-tensor in reduced Horndeski theories
• Gravitational-wave evolution of newborn magnetars with different deformed structure
• Magnetic Field Strength Effects on Nucleosynthesis from Neutron Star Merger Outflows
• Effect of the equation of state for dilute neutron matter on the composition of the inner crust of neutron stars
• Graviton-photon conversion in stochastic magnetic fields
• Cosmology in the dark: How compact binaries formation impact the gravitational-waves cosmological measurements
• Subsequent Nonthermal Emission due to the Kilonova Ejecta in GW 170817
• Proca-stinated Cosmology II: Matter, Halo, and Lensing Statistics in the vector Galileon
• Spinning gravimagnetic particles in Schwarzschild-like black holes
• Parametric amplification of electromagnetic plasma waves in resonance with a dispersive background gravitational wave
• Profiling stellar environments of gravitational wave sources
• Exploring Radial Oscillations in Slow Stable and Hybrid Neutron Stars
• Optimal Follow-Up of Gravitational-Wave Events with the UltraViolet EXplorer (UVEX)
• $g$-mode of neutron stars in pseudo-Newtonian gravity
• Triggering Electron Capture Supernovae: Dark Matter Effects in Degenerate White-Dwarf-like Cores of Super-Asymptotic Giant Branch Stars
• Higher-level large-eddy filtering strategy for general relativistic fluid simulations
• Connecting Relativistic Density Functional Theory to Microscopic Calculations
• A half-ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant
• Recent Developments in Degenerate Higher Order Scalar Tensor Theories
• Cross-Observatory Coordination with tilepy: A Novel Tool for Observations of Multi-Messenger Transient Events
• Study of hybrid stars with nonstrange quark matter cores
• Stability analysis of the spin evolution fix points in inspiraling compact binaries with black hole, neutron star, gravastar, or boson star components
• Recent astrophysical observations reproduced by a short-range correlated van der Waals-type model?
• Probing Spin-2 Ultralight Dark Matter with Space-based Gravitational Wave Detectors in the mHz Regime
• Cosmology in theories with spontaneous scalarization of neutron stars
• Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone
• Could an X-ray Flare after GRB 170817A Originate from a Post-merger Slim Accretion Disc?
• DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
• Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
• Comparison of the Origin of Short Gamma-Ray Bursts with or without Extended Emission
• Dynamically screened strongly quantized electron transport in binary neutron-star merger
• A huge-amplitude white-light superflare on a L0 brown dwarf discovered by GWAC survey
• Closed-form solutions of spinning, eccentric binary black holes at 1.5 post-Newtonian order
• Resonant Production of Light Sterile Neutrinos in Compact Binary Merger Remnants
• A novel multi-layer modular approach for real-time fuzzy-identification of gravitational-wave signals
• Effect of Dark matter and $\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• Colloquium: Multimessenger astronomy with continuous gravitational waves and future detectors
• Tidal Love Numbers of Neutron Stars in Horndeski Theories
• Probing into the Possible Range of the U Bosonic Coupling Constants in Neutron Stars Containing Hyperons
• Arm locking in conjunction with time-delay interferometry
• Pattern of lensed chirp gravitational wave signal and its implication on the mass and position of lens
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• Propagating Gravitational Waves in Teleparallel Gauss-Bonnet Gravity
• Numerical implementation of the Cubic Galileon model in PINOCCHIO
• Opportunities for Astrophysical Science from the Inner and Outer Solar System
• Suitable resolution for EOS tables in neutron star investigation
• Love-C relations for elastic hybrid stars
• Tidal Deformability as a Probe of Dark Matter in Neutron Stars
• A minimal Length Uncertainty Approach to Cosmological Constant Problem
• Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
• Constraining the $f$-mode oscillations frequency in Neutron Stars through Universal Relations in the realm of Energy-Momentum Squared Gravity
• Dynamical neutron-star tides: The signature of a mode resonance
• Effects of multidimensional treatment of gravity in simulations on supernova gravitational waves
• Methods for relativistic self-gravitating fluids: From binary neutron stars to black hole-disks and magnetized rotating neutron stars
• A search for correlated low-energy electron antineutrinos in KamLAND with gamma-ray bursts
• The origin of the coherent radio flash potentially associated with GRB 201006A
• Impact of Neutrino Flavor Conversions on Neutron Star Merger Dynamics, Ejecta, Nucleosynthesis, and Multi-Messenger Signals
• Sensing performance enhancement via asymmetric gain optimization in the atom-light hybrid interferometer
• Deciphering Accretion-Driven Starquakes in Recycled Millisecond Pulsars using Gravitational Waves
• Confronting recent light compact star observations with color-flavor locked quark matter
• Cosmological Standard Timers from Unstable Primordial Relics
• The constraint ability of Hubble parameter by gravitational wave standard sirens on cosmological parameters
• Multimessenger Astronomy with Neutrinos
• Towards optomechanical parametric instabilities prediction in ground-based gravitational wave detectors
• Superfluid dark stars
• Measuring Gravitational Wave Speed and Lorentz Violation with the First Three Gravitational-Wave Catalogs
• Limits on the Electro-Magnetic Counterpart of Binary Black Hole Coalescence at Visible Wavelengths
• The origin of the KLT relations and nonlinear relations for Yang-Mills amplitudes
• Probing Strange Dark Matter through $f$-mode Oscillations of Neutron Stars with Hyperons and Quark Matter
• Limiting the Number of Extra Dimensions with Shortcuts
• Probing the progenitor of high-$z$ short-duration GRB 201221D and its possible bulk acceleration in prompt emission
• Bifurcated symmetry breaking in scalar-tensor gravity
• New modeling for hybrid stars with an elastic quark core
• Exploring nuclear force with pulsar glitch observation
• Modeling the Multi-band Light Curves of the Afterglows of Three Gamma-Ray Bursts and Their Associated Supernovae
• Luminal Scalar-Tensor theories for a not so dark Dark Energy
• Oscillatory properties of strange quark stars described by the vector MIT bag model
• Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
• Probing black hole `charge' from the binary black hole inspiral
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Analogy of space time as un elastic medium -- Can we establish a thermal expansion coefficient of space from the cosmological constant Lambda?
• Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
• Neutron star evolution with the Bemfica-Disconzi-Noronha-Kovtun viscous hydrodynamics framework
• Transient electromagnetic sources can detect solitary black holes in Milky Way galaxy
• Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium Core$-$Black Hole Mergers Following Delayed Dynamical Instability
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Quantum Oppenheimer-Snyder models in loop quantum cosmology with Lorentz term
• Self-consistent interaction of linear gravitational and electromagnetic waves in non-magnetized plasma
• Testing Lorentz symmetry with space-based gravitational-wave detectors
• Gauge invariant perturbations in teleparallel Horndeski gravity
• Multi-messenger astronomy in the new physics modality with GPS constellation
• Ladder Symmetry: The Necessary and Sufficient Condition for Vanishing Love Numbers
• Optimizing the low-latency localization of gravitational waves
• Event Rate of Fast Radio Burst from Binary Neutron-star Mergers
• An SZ-Like Effect on Cosmological Gravitational Wave Backgrounds
• Screening fifth forces in scalar-vector-tensor theories
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
• An estimate of the gravitational-wave background from the observed cosmological distribution of quasars
• $f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
• Neutron Star in Quantized-space-time
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• An eccentric binary blackhole in post-Newtonian theory
• Axial perturbations of neutron stars with shift symmetric conformal coupling
• An Archival Search for Neutron-Star Mergers in Gravitational Waves and Very-High-Energy Gamma Rays
• Probing the Dark Solar System: Detecting Binary Asteroids with a Space-Based Interferometric Asteroid Explorer
• Strange Matter
• Effective Field Theories for Neutron Stars Physics
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• An infinite class of exact rotating black hole metrics of modified gravity
• Inflationary solutions in the simplest gravity model with conformal symmetry
• Status of the Advanced Virgo gravitational-wave detector
• Extended Gravity Constraints at Different Scales
• KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies
• Detectability of dark matter density distribution via gravitational waves from binary black holes in the Galactic center
• Quark confinement in an equiparticle quark model: application to stellar matter
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• High-energy emissions from neutron star mergers
• Neutron Star Radii from Laboratory Experiments
• Joint inference for gravitational wave signals and glitches using a data-informed glitch model
• Raychaudhuri Equation and Weyl-Driven Shear: A Weak-Field Approach to Lensing and Gravitational Waves
• FALCO: a Foundation model of Astronomical Light Curves for time dOmain astronomy
• Black hole spectroscopy of collapsing and merging neutron stars
• Bayesian analysis of multimessenger M-R data with interpolated hybrid EoS
• Dark matter effect attributed to the inherent structure of cosmic space
• Thermal behavior of a radially deformed black hole spacetime
• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
• Quasinormal Modes and Shadows of Black Holes in Infinite Derivative Theory of Gravity
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• Misaligned snowplough effect and the electromagnetic counterpart to black hole binary mergers
• Decoupled Quark Stars Relativistic Models in the Regime of Self-interacting Brans-Dicke Gravity
• Five dimensional rotating and Quintessence black hole and their hypershadows
• ComPair-2: A Next Generation Medium Energy Gamma-ray Telescope Prototype
• The R-Process Alliance: Hunting for gold in the near-UV spectrum of 2MASS J05383296-5904280
• Principal Components for Model-Agnostic Modified Gravity with 3x2pt
• Quark-Gluon Plasma and Nucleons a la Laughlin
• Delayed Thermal Relaxation of Rapidly Cooling Neutron Stars: Nucleon Superfluidity and Non-nucleon Particles
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Simulating bulk viscosity in neutron stars. I. Formalism
• Burgers equation for the bulk viscous pressure of quark matter
• Introduction to gravitational wave astronomy
• Long-term impact of the magnetic-field strength on the evolution and electromagnetic emission by neutron-star merger remnants
• Textual interpretation of transient image classifications from large language models
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• Neutron star under homotopy perturbation method
• Exploring Temperature Influences on Gravitational Wave Production in Binary White Dwarfs
• Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)
• A holographic study on QCD phase transition and neutron star properties
• Tests of Classical Gravity with Radio Pulsars
• Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
• Binary Neutron Star (BNS) merger: What we learned from relativistic ejecta of GW/GRB~170817A
• An optimal envelope ejection efficiency for merging neutron stars
• Strong NIR emission following the long duration GRB 211211A: Dust heating as an alternative to a kilonova
• Visualizing gravitational Bessel waves
• The THESEUS space mission: science goals, requirements and mission concept
• Self-calibration of Networks of Gravitational Wave Detectors
• Spacetime Curvature as a Probe of Exotic Core Phases in Neutron Stars within Modified Gravity
• Extended primordial black hole mass functions with a spike
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Constraint evolution in first-order viscous relativistic fluids
• Detecting and Diagnosing Terrestrial Gravitational-Wave Mimics Through Feature Learning
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• Gravitational scattering of two neutron stars
• Insights into Binary Neutron Star Merger Simulations: A Multi-Code Comparison
• The Impact of $f(\mathcal{G},T)$ Gravity on the Evolution of Cavity in the Cluster of Stars
• Gravitational Waves Emission in Quadratic Gravity: longitudinal modes, angular momentum emission, and positivity of the radiated power
• Impact of the relativistic Cowling approximation on shear and interface modes of neutron stars
• What to expect: kilonova light curve predictions via equation of state marginalization
• First joint observation by the underground gravitational-wave detector, KAGRA, with GEO600
• Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
• Modulations of Gravitational Waves due to Non-static Gravitational Lenses
• Hybrid stars can be self-bound
• Effects of Dark Matter on the Spontaneous Scalarization in Neutron Stars
• Neutron Star with Dark Matter Admixture: A Candidate for Bridging the Mass Gap
• Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
• Identification of Strongly Lensed Gravitational Wave Events Using Squeeze-and-Excitation Multilayer Perceptron Data-efficient Image Transformer
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Optimal collision-energy range for realizing macroscopic high-baryon-density matter
• Bounds from multi-messenger astronomy on the Super Heavy Dark Matter
• Equation of state for hyperonic neutron-star matter in SU(3) flavor symmetry
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Pulsar as a Weber detector of gravitational waves and a probe to its internal phase transitions
• From de Sitter to anti-de Sitter singularity regularization: Theory and phenomenology
• Improved Treatment of Bosonic Dark Matter Dynamics in Neutron Stars: Consequences and Constraints
• Reheating era in Gauss-Bonnet theories of gravity compatible with the GW170817 event
• Neutron stars in the generalized SU(2) Proca theory
• Radial Oscillations of Viscous Neutron Stars: Zero Diffusion Case
• Extending the short gamma-ray burst population from sub-threshold triggers in Fermi/GBM and GECAM data and its implications
• K-mouflage at high $k$: extending the reach of $\text{Hi-COLA}$
• Atmospheric Newtonian noise modeling for third-generation gravitational wave detectors
• Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes
• Population synthesis of Thorne-Żytkow objects: Rejuvenated donors and unexplored progenitors in the common envelope formation channel
• Rates and beaming angles of GRBs associated with compact binary coalescences
• Extended body dynamics in general relativity: hyperelastic models
• Gravitational glint: Detectable gravitational wave tails from stars and compact objects
• Neutrinos and Heavy Element Nucleosynthesis
• On the role of magnetic fields into the dynamics and gravitational wave emission of binary neutron stars
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Semiclassical Effects in Color Flavor Locked Strange Stars
• Deep Multimessenger Search for Compact Binary Mergers in LIGO, Virgo, and Fermi/GBM Data from 2016-2017
• A Very-High-Energy Gamma-Ray View of the Transient Sky
• All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
• On non-detection of Gamma-Ray Bursts in three compact binary merger events detected by LIGO
• Unstable modes of hypermassive compact stars driven by viscosity and gravitational radiation
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Gravitational waves in gauge theory gravity with a negative cosmological constant
• Some geometrical aspects of gravitational waves using continuum mechanics analogy: State of the art and potential consequences
• Gravitational Wave Emission from Close-in Strange Quark Planets Around Strange Stars with Magnetic Interactions
• Double neutron star formation via consecutive type II supernova explosions
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Exploring the Orbital Alignments of Galactic Close White Dwarf Binaries with LISA
• A Post-Newtonian Analysis of Regularized 4D-EGB Theory: Complete Set of PPN Parameters and Observational Constraints
• Thermodynamic topology of dyonic AdS black holes with quasitopological electromagnetism in Einstein-Gauss-Bonnet gravity
• Off-axis MeV and very-high-energy gamma-ray emissions from structured gamma-ray burst jets
• Deriving Neutron Star Equation of State from AdS/QCD
• Revealing the elusive companion of the red giant binary 2MASSJ05215658+4359220 from UV HST and Astrosat-UVIT data
• PPN meets EFT of dark energy: Post-Newtonian approximation in higher-order scalar-tensor theories
• Constraints on the internal physics of neutron stars from the observational data of several young pulsars: the role of a power-law decaying dipole magnetic field
• Scalarized non-topological neutron stars in multi-scalar Gauss-Bonnet gravity
• Dense Hadronic Matter in Neutron Stars
• Enhancing high frequency sensitivity of gravitational wave detectors with sloshing-Sagnac interferometer
• Is warm inflation quasi-stable?
• Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations
• Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework
• Testing black hole metrics with binary black hole inspirals
• Toward Cosmological Standard Timers in Primordial Black Hole Binaries
• Analogy of space-time as an elastic medium -- Study of the perturbation tensor of the metric $h_{\mu \nu }$ through the prism of the analogy of the theory of elasticity -- Analysis and potential consequences
• Displacement-noise-free interferometeric gravitational-wave detector using unidirectional neutrons with four speeds
• Shared Properties of Merger-driven Long-duration Gamma-Ray Bursts
• A constraint on superheavy elements of the GRB-kilonova AT 2023vfi
• Gravitational dynamics in a 2+1+1 decomposed spacetime along nonorthogonal double foliations: Hamiltonian evolution and gauge fixing
• Detecting milli-Hz gravitational waves with optical resonators
• Finite-temperature equation of state with hyperons
• Rapid Hierarchical Inference of Neutron Star Equation of State from multiple Gravitational Wave Observations of Binary Neutron Star Coalescences
• The impact of rare events on the chemical enrichment in dwarf galaxies
• Type I Shapovalov wave spacetimes in the Brans-Dicke scalar-tensor theory of gravity
• Gravitational wave signatures of phase transition from hadronic to quark matter in isolated neutron stars and binaries
• Effect of symmetry energy on properties of rapidly rotating neutron stars and universal relations
• Nonminimal Derivative Coupling Cosmology and the Speed of Gravitational Waves
• How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal
• Low-frequency gravitational wave memory from gamma-ray burst afterglows with energy injection
• Diquarkyonic matter: quarks, diquarks and baryons
• Gravitational Waves and Electromagnetic Transients
• Novel black holes with scalar hair in the Einstein-Maxwell-Scalar Theory with positive coupling
• Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks
• A long-duration gamma-ray burst of dynamical origin from the nucleus of an ancient galaxy
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Can a hybrid star with constant sound speed parametrization explain the new NICER mass-radius measurements ?
• Cosmological memory effect in scalar-tensor theories
• A single-atom level mechano-optical transducer for ultrasensitive force sensing
• Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
• On the stability of covariant BSSN formulation
• Multimessenger Probes of High-energy Sources
• Hot and highly magnetized neutron star matter properties with Skyrme interactions
• Quantum gravity phenomenology from the perspective of quantum general relativity and quadratic gravity
• Boosting the Efficiency of Parametric Detection with Hierarchical Neural Networks
• Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals
• Gravitational decoherence: a non relativistic spin 1/2 fermionic model
• Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star
• Gravitational Waves from Strange Star Core-Crust Oscillation
• Implementation of the rROF denoising method in the cWB pipeline for gravitational-wave data analysis
• Correlation between the curvature and some properties of the neutron star
• Dynamical hair growth in black hole binaries in Einstein-scalar-Gauss-Bonnet gravity
• Spin and quadrupolar effects in the secular evolution of precessing compact binaries with black hole, neutron star, gravastar, or boson star components
• Sensing and control scheme for the inteferometer configuration with an L-shaped resonator
• Characterization of the inner edge of the neutron star crust
• GRB 180728A and SN 2018fip: the nearest high-energy cosmological gamma-ray burst with an associated supernova
• MUPHOTEN : a MUlti-band PHOtometry Tool for TElescope Network
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Search for gravitational-neutrino correlations on ground-based detectors
• Probing the equation of state of neutron stars with captured primordial black holes
• Neutron star oscillations in pseudo-Newtonian gravity
• Hybrid stars from a constrained equation of state
• Binary neutron star mergers within kaon condensation: GW170817
• Universal relations between the quasinormal modes of neutron stars and magnetic tidal deformability
• Machine-directed gravitational-wave counterpart discovery
• Space-based Gravitational Wave Observatories
• The Role of r-Modes in Pulsar Spin-down, Pulsar Timing, and Gravitational Waves
• Astrophysical constraints on the cold equation of state of the strongly interacting matter
• Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Skyrme-based extrapolation for the static response of neutron matter
• Notes on primordial black hole origin for thermal gamma-ray bursts
• Wald Entropy in Extended Modified Myrzakulov Gravity Theories: \(f(R, T, Q, R_{μν}T^{μν}, R_{μν}Q^{μν}, \dots)\)
• Bubble dynamics in the Polyakov quark-meson model
• Antineutrino Opacity in Neutron Stars in the Models Constrained by Recent Terrestrial Experiments and Astrophysical Observations
• Metric Assisted Stochastic Sampling (MASS) search for gravitational waves from binary black hole mergers
• Modelling the chemical evolution of the Milky Way
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Linear and nonlinear clusterings of Horndeski-inspired dark energy models with fast transition
• Solar System Experiments in the Search for Dark Energy and Dark Matter
• Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers
• Bose-Einstein Condensate and Liquid Helium He${}^4$: Implications of GUP and Modified Gravity Correspondence
• Scalarized neutron stars with a highly relativistic core in scalar-tensor gravity
• El-CID: A filter for Gravitational-wave Electromagnetic Counterpart Identification
• How Do Nuclear Isomers Influence the Gamma-Ray Bursts in Binary Neutron Star Mergers?
• Higher order mimetic gravity after GW170817
• Gravitational-Wave Constraints on Neutron-Star Pressure Anisotropy via Universal Relations
• Hairy black holes in extended Einstein-Maxwell-scalar theories with magnetic charge and kinetic couplings
• A Bayesian Inference Framework for Gamma-Ray Burst Afterglow Properties
• Light Travel Time Effects in Kilonova Models
• Dynamical ejecta of neutron star mergers with nucleonic weak processes I: Nucleosynthesis
• Shear viscosity in QCD and why it's hard to calculate
• Exploring the connection between compact object mergers and fast X-ray transients: The cases of LXT 240402A and EP250207b
• Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
• $f$-mode oscillations of compact stars with realistic equations of state in dynamical spacetime
• Merged white dwarfs and nucleosynthesis
• Tidal reconstruction of neutron star mergers from their late inspiral
• An Online Framework for Fitting Fast Transient Lightcurves
• Binary black holes in magnetized AGN disks
• Bayesian inference favors quark matter in neutron star interiors
• Bayesian Analysis of Wave-Optics Gravitationally Lensed Massive Black Hole Binaries with Space-Based Gravitational Wave Detector
• Effect of spin in binary neutron star mergers
• A new experiment for the gravitational waves detection
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• On phenomenological parametrizations for the luminosity distance of gravitational waves
• Role of particle diffusion in shaping the gravitational wave signal from neutron star inspirals
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Stellar response after stripping as a model for common-envelope outcomes
• General relativistic hydrodynamic simulations of binary strange star mergers
• Four no-go theorems on the existence of spin and orbital angular momentum of massless bosons
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Enhancing gravitational-wave host localization with SKYFAST: rapid volume and inclination angle reconstruction
• Sound Speed Resonance of Gravitational Waves in Gauss-Bonnet-coupled inflation
• Analysis of critical parameters for nonrelativistic models in symmetric nuclear matter
• Gravitational and electromagnetic perturbations of a charged black hole in a general gauge condition
• Features and prospects for kilonova remnant detection with current and future surveys
• On the Gravitational Wave Counterpart to a Gamma-ray Galactic Center Signal from Millisecond Pulsars
• Search for a Gravitational-Wave Background from Sound Speed Resonance from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey
• Follow-up of Neutron Star Mergers with CTA and Prospects for Joint Detection with Gravitational-Wave Detectors
• SMASH as an event generator for heavy-ion collisions
• Echoes and quasinormal modes of asymmetric black bounces
• A way of decoupling the gravitational bulk field equations of regular braneworld black holes to suppress the bulk singularities
• Chemical enrichment by collapsars as the origin of the unusually high [Ba/Fe] in a massive star cluster of the dwarf galaxy NGC 1569
• GRBs luminosity function synthesized from \textit{Swift/BAT}, \textit{Fermi/GBM} and \textit{Konus-Wind} data
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• Signatures of secondary acceleration in neutrino flares
• Light-like shockwaves in scalar-tensor theories
• Gravitational waves in Hořava-Lifshitz anisotropic gravity
• Long-Range Quantum Gravity
• Can Neutron Star Tidal Effects Obscure Deviations from General Relativity?
• RADAR-Radio Afterglow Detection and AI-driven Response: A Federated Framework for Gravitational Wave Event Follow-Up
• Synchronized neutrino communications over intergalactic distances
• Probing small neutron skin variations in isotope pairs by hyperon-antihyperon production in antiproton--nucleus interactions
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• Magnetohydrodynamic waves excited by a coupling between gravitational waves and a strongly magnetized plasma in binaries of neutron stars
• Star Log-extended eMulation: a method for efficient computation of the Tolman-Oppenheimer-Volkoff equations
• Equation of State of Decompressed Quark Matter, and Observational Signatures of Quark-Star Mergers
• Accurate flux calibration of GW170817: is the X-ray counterpart on the rise?
• Gravitational Lensing in the Kerr Spacetime: An Analytic Approach for Light and High-Frequency Gravitational Waves
• Multi-Messenger Astrophysics with THESEUS in the 2030s
• Using t-SNE for characterizing glitches in LIGO detectors
• General relativistic hydrodynamics code for dynamical spacetimes with curvilinear coordinates, tabulated equations of state, and neutrino physics
• Astro- and Quantum Physical Tests of Screened Scalar Fields
• The Supersonic Project: SIGOs, a Proposed Progenitor to Globular Clusters, and their Connections to Gravitational Wave Anisotropies
• Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials
• Elliptically Polarized Plane Gravitational Waves
• Dynamical Shortcomings in the Generalized SU(2) Proca Theory: Challenges for Cosmic Acceleration
• Macroscopic properties of the XTE J1814-338 as a dark matter admixed strange star
• Sky localization of gravitational waves from eccentric binaries
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• Fast Generation of Weak Lensing Maps in Modified Gravity with COLA
• A Neutron Star with a Strange Quark Star-like Mass-Radius Relation
• Modeling the emission lines from r-process elements in Supernova nebulae
• Joint estimation of the cosmological model and the mass and redshift distributions of the binary black hole population with the Einstein Telescope
• Neutrino Energy Loss Rates in 3-3-1 Models
• Comment on "Testing claims of the GW170817 binary neutron star inspiral affecting $\beta$-decay rates''
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• Black hole solutions in Cotton gravity coupled to nonlinear electrodynamics
• Scalar-induced gravitational waves in spatially covariant gravity
• Dipole Polarizability of Finite Nuclei as a Probe of Neutron Stars
• Energy release from magnetospheres deformed by gravitational waves
• Plasma Instabilities Dominate Radioactive Transients Magnetic Fields: The self-confinement of leptons in Type Ia and Core-Collapse Supernovae, and Kilonovae
• A post-Newtonian approach to neutron star oscillations
• Convenient filtering techniques for LIGO strain of the GW150914 event
• Note on neutron star equation of state in the light of GW170817
• Wave zone in the Hořava-Lifshitz theory at the kinetic-conformal point in the low energy regime
• Fully general-relativistic simulations of isolated and binary strange quark stars
• Detection probability of light compact binary mergers in future observing runs of the current ground-based gravitational wave detector network
• Imprints of Non-Symmetric Dark Matter Halos on Magnetars: A Two-Fluid Perspective
• In-medium $\Delta (1232)$ potential, pion production in heavy-ion collisions and the symmetry energy
• Piecewise polytropic meshing and refinement method for the reconstruction of the neutron star equation of state using tidal deformabilities and constraints in the piecewise polytropic parameters given by the GW170817 event
• Looking for ancillary signals around GW150914
• Complete Catalog of Laser Locking Configurations for LISA
• Bulk Viscosity of Two-Flavor Color Superconducting Quark Matter in Neutron Star Mergers
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• Revisiting Flat Rotation Curves in Chern-Simons Modified Gravity
• Searches for beyond-standard-model physics with astroparticle physics instruments
• Targeted optimization in small-scale atomic structure calculations: application to Au I
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• Glitches far from transient gravitational-wave events do not bias inference
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• Evolutionary tracks of binary neutron star progenitors across cosmic times
• Absorption and scattering of massless scalar waves by black holes in quasi-topological gravity
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• The role of equation of state on the spin-up of millisecond pulsars
• Development of a polarimetry method toward in-situ substrate birefringence characterization of ground-based gravitational wave detectors
• Dynamical Casimir effect and the possibility of laser-like generation of gravitational radiation
• A Proposal for a Fast Infrared Bursts Detector
• Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts
• A quantisation procedure in the presence of an initial Kasner singularity: primordial gravitational waves from triaxially anisotropic pre-inflation
• Influence of hyperon-hyperon interaction on the properties of neutron stars
• Effects of the symmetry energy slope on magnetized neutron stars
• Quadratic theory of gravity with a scalar field and type I Shapovalov wave spacetimes
• Bounce Cosmologies in Generalized Coupling Theories
• New ab initio constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: II. Thermal response in the suprasaturation density domain
• Gravitational ringdown in the Minimal Theory of Massive Gravity
• Locally Rotationally Symmetric Spacetimes in Einstein-Cartan Theory and Their Classification
• Neutron star evolution by combining discontinuous Galerkin and finite volume methods
• Complementary signatures of $\alpha -$attractor inflation in CMB and cosmic string Gravitational Waves
• Scattered light reduction in Sagnac Speed Meters with Tunable Coherence
• Application of Non-Linear Noise Regression in the Virgo Detector
• Monopole Excitation and Nuclear Compressibility: Present and Future Perspectives
• A ${\chi }^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences
• Effects of a Brueckner-Hartree-Fock-corrected effective mass on speed of sound, conformality, and observables of dark matter-admixed neutron stars
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach
• The chiral phase transition and equation of state in the chiral imbalance
• Neutrinos in colliding neutron stars and black holes
• Gauge invariant perturbations of $F(T,T_G)$ Cosmology
• Prospects for the detection of transient neutrino sources with PLEnuM
• Testing modified (Horndeski) gravity by combining intrinsic galaxyalignments with cosmic shear
• Neutrino oscillation in the presence of background classical sources
• Relativistic excitation of compact stars
• Testing for a Random Walk Structure in the Frequency Evolution of a Tone in Noise
• Reconstruction of Gravitational Form Factors using Generative Machine Learning
• Tidally induced multipole moments of a nonrotating black hole vanish to all post-Newtonian orders
• Equations of motion for compact binary systems in general relativity: Do they depend on the bodies' internal structure at the third post-Newtonian order?
• Quasinormal Modes from EFT of Black Hole Perturbations in Vector-Tensor Gravity
• A dynamical dark energy solution to Hubble-Lemaître tension in the light of the multimessenger era
• Inferring kilonova ejecta photospheric properties from early blackbody spectra
• Measurement of the central Galactic black hole by extremely large mass-ratio inspirals
• Scalable matched-filtering pipeline for gravitational-wave searches of compact binary mergers
• Astrophysical constraints on neutron star $f$-modes with a nonparametric equation of state representation
• The Near-Ultraviolet eXplorer (NUX): a ground-based wide-field near-UV telescope to search for near-UV transients
• Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?
• Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
• Conditional Autoencoder for Generating Binary Neutron Star Waveforms with Tidal and Precession Effects
• Peak energy--Isotropic Luminosity Correlation and Jet Opening Angle Evolution in Swift-BAT Short GRBs with Soft Tail Emission
• Symplectic quantization of multi-field Generalized Proca electrodynamics
• Mechanical Characterisation of Silicon for the ETpathfinder Test Masses
• Challenging a binary neutron star merger interpretation of GW230529
• Significant challenges for astrophysical inference with next-generation gravitational-wave observatories
• The Response of Optical Fibres to Gravitational Waves
• Effect of nonlinear electrodynamics on polarization distribution around black hole
• Parametric resonance in abelian and non-abelian gauge fields via space-time oscillations
• Spatial Curvature and Large Scale Lorentz Violation
• Studying the radiation of a white dwarf star falling onto a black hole
• Properties of rotating neutron stars in light of binary compact object mergers
• Stellar modeling within regularized 4D Einstein-Gauss-Bonnet gravity in light of current astrophysical constraints
• Electron-Ion Temperature Ratio in Transrelativistic Unmagnetized Shock Waves
• Gravitational waves in metric-affine bumblebee gravity
• Quadrupole perturbations of slowly spinning Ellis-Bronnikov wormholes
• Dark energy constraints in light of theoretical priors
• Eikonal gravitational-wave lensing in Einstein-aether theory
• A Novel Optical Design for Wide-Field Imaging in X-ray Astronomy
• Hot Holographic 2-flavor Quark Star
• Charged traversable wormholes: charge without charge
• Matter-antimatter asymmetry in generalized coupling theories
• Localized five-dimensional rotating brane-world black hole Analytically Connected to an to an AdS${}_5$ boundary
• Onset of dark energy from cosmological scalarization and gravitational wave speed
• Long-term evolution of a supernova remnant hosting a double neutron star binary
• Challenging theories of gravitation: dark matter, compact objects and gravitational waves
• Gravity from the Determinant of the Energy-Momentum: Astrophysical Implications
• Quantum point particle approximation of spinning black holes and compact stars
• Simulation Study on Constraining GW Propagation Speed by GW and GRB Joint Observation on Binary Neutron Star Mergers
• Could the stochastic gravitational wave background from newborn magnetars be detected by the advanced LIGO and Einstein Telescope?
• Proton-rich production of lanthanides: the $\nu i$ process
• Modeling of optical scattering from topographic surface measurements of high-quality mirrors
• Elastic Scattering of Cosmological Gravitational Wave Backgrounds: Primordial Black Holes and Stellar Objects
• Gravitational-wave echoes from spinning exotic compact objects: numerical waveforms from the Teukolsky equation
• Absence of gravitational polarization mechanism in the canonical bimetric theory
• Neutrino propagation in winds around the central engine of sGRB
• Accelerating gravitational-wave parameterized tests of General Relativity using a multiband decomposition of likelihood
• Ultra-compact X-ray Binaries: A Review
• Post-Newtonian Gravitational Waves with cosmological constant $\Lambda$ from the Einstein-Hilbert theory
• Kilonova Light Curve Parameter Estimation Using Likelihood-Free Inference
• Deciphering signatures of Kerr-Sen black holes in presence of plasma from the Event Horizon Telescope data
• A Mass-Shell Model of Compact Binary Coalescence
• Calculation of the transport coefficients in neutron star
• Can the phase of radiation pressure fluctuations be flipped in a single path for laser interferometric gravitational wave detectors?
• Distribution of Europium in The Milky Way Disk; Its Connection to Planetary Habitability and The Source of The R-Process
• Radial Oscillations of Viscous Stars
• Quantum sensing of high-frequency gravitational waves with ion crystals
• Outer Solar System spacecraft to probe the $\mu$Hz gravitational wave frontier
• Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia
• Cosmic expansion history analysis with Hubble parametrization in $Q^n$ gravity
• Beta-decay formulas revisited (I): Gamow--Teller and spin-dipole contributions to allowed and first-forbidden transitions
• Interacting quark matter effects on the structure of compact stars
• General relativistic magnetohydrodynamics simulations for binary neutron star mergers
• A New Search Pipeline for Short Gamma Ray Bursts in Fermi/GBM Data -- A 50% Increase in the Number of Detections
• Addressing the problem of the LIGO-Virgo-KAGRA visibility in the scientific literature
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Perturbations of Einstein--Maxwell--phantom spacetime: Instabilities of charged Ellis--Bronnikov wormholes and quasinormal modes of black holes
• Alpha clustering in warm and dense nuclear matter from heavy-ion collisions
• Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
• Electric dipole polarizability of neutron rich nuclei
• Shadow of topologically charged rotating braneworld black hole
• Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars?
• Kilonova and progenitor properties of merger-driven gamma-ray bursts
• Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments
• Constraining the competition between the deconfinement and chiral phase transitions in light of the multimessenger era
• Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade
• From Cosmic Matter to the Laboratory
• Landau parameters and entrainment matrix of cold stellar matter: effect of the symmetry energy and strong magnetic fields
• Critical masses and numerical computation of massive scalar quasinormal modes in Schwarzschild black holes
• Gravitational wave propagation in bigravity in the late universe
• Low-vibration cryogenic test facility for next generation of ground-based gravitational-wave observatories
• First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis
• Characterization of the seismic field at Virgo and improved estimates of Newtonian-noise suppression by recesses
• Can we detect the quantum nature of weak gravitational fields?
• Searching for new physics during gravitational waves propagation
• Misidentification of Short GRBs as Magnetars in Nearby Galaxies
• Horndeski in motion
• Accessing the Host Galaxies of Long Gamma-Ray Bursts with Next-Generation Telescopes
• Gravitational waves from equatorially eccentric extreme mass ratio inspirals around swirling Kerr black holes
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• Axion Dark Matter Archaeology with Primordial Gravitational Waves
• Impact of hyperons on structural properties of neutron stars and hybrid stars within the regularized four-dimensional Einstein-Gauss-Bonnet gravity
• Jet-environment interaction after delayed collapse in binary neutron star mergers
• A Cosmological Bragg Law: Interpreting the CMB as a Diffractogram of Foliated Spacetime
• Benford's law in atomic spectra and opacity databases
• Radio astronomy and Space science in Azores: enhancing the Atlantic VLBI infrastructure cluster
• Early Detection of Multiwavelength Blazar Variability
• Tidal deformations of compact objects and gravitational wave emission
• Modeling Neutron Star Oscillations in a Fixed General Relativistic Background Including Solid Crust Dynamics
• A Fundamental Plane in X-ray Binary Activity of External Galaxies
• Prospects for High-Frequency Gravitational-Wave Detection with GEO600
• Maximal mass of the neutron star with a deconfined quark core
• Compact binary system dynamics at the second post-Newtonian order: analytical formula of the coordinate time for eccentric and circular orbits
• Harvesting entanglement from the cylindrical gravitational wave spacetime
• Bounding dark charges on binary black holes using gravitational waves
• Efectos del campo magnético en un gas de bosones vectoriales neutros: aplicaciones astrofísicas
• Infrared Sensitivity of Cosmological Probes in Horndeski Theory
• Glitch veto based on unphysical gravitational wave binary inspiral templates
• Electron impact excitation of Te IV and V and Level Resolved R-matrix Photoionization of Te I - IV with application to modelling of AT2017gfo
• BHaHAHA: A Fast, Robust Apparent Horizon Finder Library for Numerical Relativity
• Multivariate Time Series Clustering for Environmental State Characterization of Ground-Based Gravitational-Wave Detectors
• Gravitational waves from sub-solar mass primordial black holes
• Approaching ballistic motion in 3D simulations of gamma-ray burst jets in realistic binary neutron star merger environments
• Exploring Hyperon Skyrme Forces in Multi-$\Lambda$ Hypernuclei and Neutron Star Matter
• Towards asteroseismology of neutron stars with physics-informed neural networks
• Quasi-universality of the magnetic deformation for neutron stars in general relativity and beyond
• Mass Oscillations in Superconducting Junctions for Gravitational Wave Emission and Detection
• Numerical simulations of oscillating and differentially rotating neutron stars
• Neutron stars as extreme gravity probes
• Kilohertz Gravitational Waves from Binary Neutron Star Mergers: Full Spectrum Analyses and High-density Constraints on Neutron Star Matter
• Identifying the QCD Phase Transitions via the Gravitational Wave Frequency from Supernova Explosion
• Does a long-lived remnant neutron star exist after short gamma-ray burst GRB 160821B?
• Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• Constraints from the GW170817 merger event on the nuclear matter equation of state
• Expanding the Population of Short Gamma-Ray Transients with a Coherent Fermi/GBM Search. A 13-year catalog of short GRBs
• Calibrating systematic errors in the distance determination with the luminosity-distance space large scale structure of dark sirens and its potential applications
• Gravitational waveforms from inspiral compact binaries in Hybrid metric-Palatini gravity
• Image of a quantum-corrected black hole without Cauchy horizons illuminated by a static thin accretion disk
• Thermal aspects of neutron star mergers
• Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
• Constraining the quantum gravity polymer scale using LIGO data
• Characterizing the quark-hadron mixed phase in compact star cores : sensitivity to nuclear saturation and quark-model parameters at finite-temperature
• Constraining the abundance of spinning deformed Galactic compact objects with continuous gravitational waves
• The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles
• Matters of Gravity, The Newsletter of the Division of Gravitational Physics of the American Physical Society, Volume 48, December 2016
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Neutron Stars in Causal Scalar-Tensor Theories
• Astronomy and the new SI
• Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
• Collapsing domain walls with ${\mathbb{Z}}_2$-violating coupling to thermalized fermions and their impact on gravitational wave detections
• Scattering Amplitudes for Binary Systems beyond GR
• Exploring Composition Mixing in Kilonova Ejecta with Ray-by-ray Simulations
• Adding Gamma-ray Polarimetry to the Multi-Messenger Era
• Quantum matter and gravitation: photons in a waveguide
• First-post-Newtonian generation of gravitational waves in Einstein-Cartan theory
• Ringing Black Hole is Superradiant: Ultra-light Scalar Field
• A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar?
• Detection of a Millisecond Periodicity in BATSE Short Gamma-Ray Bursts
• Gravitational wave interactions with a viscous fluid: Core collapse supernova, binary neutron star merger, and accretion around a black hole merger
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars : Spinning case
• An alternative statistical interpretation for the apparent plateaus in the duration distributions of GRBs
• EFT of Dark Energy with Cosmic Chronometers: Reconstructing Background EFT Functions
• The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
• Analytical solutions of bound timelike geodesic orbits in effective-one-body frame
• Revisiting black hole hyperaccretion in the center of gamma-ray bursts for the lower mass gap
• Soliton boson stars, Q-balls and the causal Buchdahl bound
• Search for Periodic Radio Signals from Double Neutron Star System Companions Using the Fast Folding Algorithm
• Linear perturbations of dyonic black holes in the lowest-order $U(1)$ gauge-invariant scalar-vector-tensor theories
• Signatures of deconfined quark phases in binary neutron star mergers
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Impact of Anisotropy on Neutron Star Structure and Curvature
• Effective-one-body formalism for leading-order radiative effects in the post-linear framework
• Scrambling time for analogue black holes embedded in AdS space
• Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
• Gravitational waves in Cubic Metric-Affine Gravity
• Similar Fermi-GBM sGRBs to GW/sGRB 170817A in MeV-GeV energies
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Influences of parametrizations of density dependent couplings
• New mass estimates for massive binary systems: a probabilistic approach using polarimetric radiative transfer
• Macroscopic backreaction of the trace anomaly on classical vacuum backgrounds
• The stochastic gravitational wave background from magnetars
• EFPE: Efficient fully precessing eccentric gravitational waveforms for binaries with long inspirals
• Toward a Unified Understanding of the Dense Matter Equation of State
• Tracing the Trace Anomaly of Dense Matter inside Neutron Stars
• Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers
• Gravitational Bound State Perturbations Inside Black Holes and Isospectrality
• Topological Shell Structures in Neutron Stars: Effects on Equilibrium, Oscillations, and Gravitational-Wave Signatures
• Spectral Hardness as the Primary Discriminator: Unveiling the Collapsar--Merger Boundary with a Gold-Standard Gamma-Ray Burst Sample
• Gravitational lensing of Continuous Gravitational Waves
• Unitary time-evolution in stochastic time-dependent Hilbert spaces
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• Heavy-ion collision simulation with high performance computer
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• Tidal love number of neutron stars with conformal coupling
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• Design of a tabletop interferometer with quantum amplification
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• The Parallel Compact Object CALculator: An Efficient General Relativistic Initial Data Solver for Compact Objects
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• Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
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• Applying models of pulsar wind nebulae to explain X-ray plateaux following short gamma-ray bursts
• Cavendish experiment with fast radio bursts on cosmological scales
• Alternative LISA-TAIJI networks: detectability of the isotropic stochastic gravitational wave background
• Light scalars in neutron star mergers
• Rising Tides: Analytic Modeling of Tidal Effects in Binary Neutron Star Mergers
• In situ substrate birefringence characterization in gravitational wave detectors using a heterodyne polarimetry method
• Gravitational background from dynamical binaries and detectability with 2G detectors
• Detecting White Dwarf Binary Mergers with Gravitational Waves
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• Interferometric sensing of a commercial geophone
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• Linear perturbations of Kerr black hole in quadratic gravity
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• The nuclear matter density functional under the nucleonic hypothesis
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• SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO-Virgo Event GW190814
• Searching For Strange Quark Planets
• FRB 121102: a star quake-induced repeater?
• Probing cosmology with bright sirens from the CosmoDC2_BCO LSST synthetic catalog
• Gamma-ray Bursts
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• Are Interactions with Neutron Star Merger Winds Shaping the Jets?
• Universal relation between dipole polarizability of finite nuclei and neutron-star compactness
• Multimodal analysis of Gravitational Wave signals and Gamma-Ray Bursts from binary neutron star mergers
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Unifying gravitational waves and dark energy
• Enhancing online estimation of CBC parameters with the low-latency MBTA analysis
• Detectability of continuous gravitational waves from planetary-mass companions orbiting compact stars
• Mass-radius relation, moment of inertia, and tidal love numbers of anisotropic neutron stars in f (R,T) gravity
• Systematic study for the surface properties of neutron star
• Effects of anisotropy on strongly magnetized neutron and strange quark stars in general relativity
• Rotation-dependent $I$-Love-$Q$-$\delta M$ relations in perturbation theory
• Light curves and polarizations of gravitationally lensed kilonovae
• Neutrino mean free path in neutron stars in the presence of hyperons
• Gravitational wave seismology of charged strange stars in the Cowling approximation: the fluid pulsation modes
• Recent advances on multimessenger astrophysics: Centaurus A, GW 170817, and KM3-230213A
• Design and preliminary performance study of the broad-band spectrometer detector for POLAR-2
• Hybrid stars with large strange quark cores
• Universality of the halo mass function in modified gravity cosmologies
• Quantum Physics in Space
• P-stars in the gravitational wave era
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• Testing the Non-circularity of the Spacetime around Sagittarius A* with Orbiting Pulsars
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Investigating the mass-ratio dependence of the prompt-collapse threshold with numerical-relativity simulations
• Outliers in spectral time lag selected gamma-ray bursts
• Unveiling gravitational waves from core-collapse supernovae with MUSE
• Graviton Photoproduction by a Kerr-Newman Black Hole with Worldline EFT
• A Robust and Efficient F-statistic-based Framework for Consistent Bayesian Inference of Compact Binary Coalescences
• Constraining Hamiltonians from chiral effective field theory with neutron-star data
• Gravitational waves from spinning neutron stars as not-quite-standard sirens
• Local energy density functional for superfluid Fermi gases from effective field theory
• Differentiating between sharp and smoother phase transitions in neutron stars
• Gravitational-Wave Signatures of Massive Black Hole Formation
• Tidal effect on the gyroscopic precession around a compact star
• Quantum phase estimation with optimal confidence interval using three control qubits
• Evaluation of microseismic motion at the KAGRA site based on ocean wave data
• Preliminary results of the pixel characterization for the Crystal Eye, a new X and gamma-ray satellite detector for multi-messenger astronomy
• Astrometric microlensing probes of the isolated neutron star population with Roman
• Lie Group Theory of Multipole Moments and Shape of Stationary Rotating Fluid Bodies
• A Census of Sun's Ancestors and their Contributions to the Solar System Chemical Composition
• Constraining the Time of Gravitational Wave Emission from Core-Collapse Supernovae
• Compact elastic objects in general relativity
• Residual neural networks to classify the high frequency emission in core-collapse supernova gravitational waves
• Relativistic star solutions in Mass-varying Massive Gravity with a diagonal metric
• On the use of CHIME to Detect Long-Duration Radio Transients from Neutron Star Mergers
• Asymptotic Freedom and Vacuum Polarization Determine the Astrophysical End State of Relativistic Gravitational Collapse: Quark--Gluon Plasma Star Instead of Black Hole
• GW170817 and GW190814: tension on the maximum mass
• Gamma-radiation sky maps from compact binaries
• Light rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories
• Population Properties of Binary Black Holes with Eccentricity
• New effective theories of gravitation and their phenomenological consequences
• What are neutron stars made of? Gravitational waves may reveal the answer
• Generalized Linear Models of T${}_{90}$-T${}_{50}$ relation to classify GRBs
• Hybrid star properties from an extended linear sigma model
• Isospin blocking and its effects in heavy-ion collisions
• Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
• Strong field gravitational lensing of particles by a black-bounce-Schwarzschild black hole
• Scalar-Induced Gravitational Waves in Palatini $f(R)$ Gravity
• Superradiant scattering of massive scalar field due to magnetically charged rotating black hole
• Connections between entropy surface density and microscopic property in black holes
• Universality of the Blandford-Znajek emission in stationary and axisymmetric spacetimes
• Neutron Stars in Scalar Torsion Theories with Nonminimal Coupling
• Investigating Universal Relations in Compact Stars featuring $\Delta -$Admixed Exotic Dense Matter
• Stability Analysis of Four $f(Q)$ Gravity Models : A Cosmological Review in the Background of Bianchi-I Anisotropy
• The gravitational waves from the collapsing domain walls in the complex singlet model
• Circularly polarized gravitational waves from parity-violating scalar-tensor theory
• Photon Ring Dimming as a Signature of Photon-Axion Conversion in Janis-Newman-Winicour Naked Singularity
• Topological dressing method for the Einstein-Maxwell equations
• Linear perturbations of an exact gravitational wave in the Bianchi IV universe
• Radial perturbations of scalar-Gauss-Bonnet black holes beyond spontaneous scalarization
• Dense Baryonic Matter and Applications of QCD Phase Diagram Dualities
• Constraining the Nuclear Equation of State from Rotating Neutron Stars
• Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• Preliminary census of galaxies in the LISA localisation volume: I. Searching for LISA candidate massive black hole binary merger hosts using Sloan Digital Sky Survey photometry
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• The impact of kilonova seed photons on GRB VHE emission
• Three-dimensional equation of state extension of quark matter in Fermi-liquid theory
• Searching for gravitational waves from compact binary mergers powering long gamma-ray bursts during LIGO-Virgo-KAGRA's O3 run
• Random projections in gravitational-wave searches from compact binaries II: efficient reconstruction of the detection statistic
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Impact of crust-core connection procedures on the tidal deformability of neutron stars
• Estimating source distances for high-energy neutrinos: A method for improving electromagnetic follow-up searches
• Constraining Binary Neutron Star Populations using Short Gamma-Ray Burst Observations
• Constraints on the Neutron Star Equation of State from GW170817
• An introduction to astrophysical observables in gravitational wave detections
• Incorporating a radiative hydrodynamics scheme in the numerical-relativity code BAM
• Resonant Axion-Photon Conversion in the Early Inspiral of Neutron Star Binaries
• Inferring binary black holes stellar progenitors with gravitational wave sources
• General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars
• Kinematic Evidence for Open Cluster Origins of Galactic Binary Neutron Stars
• Predicting Angular-Momentum Waves Based on Yang-Mills Equations
• GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B
• Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
• Gravitational wave memory in wormhole spacetimes
• Even parity potential for spacetimes with Gaussian matter source and its associated QNM spectra
• High Sensitivity Methodologies to Detect Radio Band Gravitational Waves
• $\gamma$ rays run on time
• Measurement of High Energy Gamma Rays from 200 MeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
• Scattering from compact objects: Debye series and Regge-Debye poles
• Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• The Completeness of Accreting Neutron Star Binary Candidates from the Chinese Space Station Telescope
• A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• The Gravito-Phononic Effect: A Quantum Signature of Linearised Gravity
• Holography in Quark-Gluon Plasma and Neutron Stars
• Investigating the effects of gravitational lensing by Hu-Sawicki $\mathbf{f}(\mathbf{R})$ gravity black holes
• Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes
• Stochastic gravitational wave background due to core collapse resulting in neutron stars
• Constraining the Phase-Transition EoS using the Energy Dependence of Directed Flow
• Cluster gravitational redshifts: uncertainties and survey requirements
• Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description
• Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
• Eccentricity reduction of binary neutron star initial data with the entropy based flux limiting scheme
• Novae breves from magnetar giant flares: Potential probes of neutron star crusts
• A dual description of quarks and baryons: Quarkyonic matter within a relativistic quark model
• Electron wave functions in beta-decay formulas revisited (II): Completion including recoil-order and induced currents
• Constraining gravitational wave velocities using gravitational and electromagnetic wave observations of white dwarf binaries
• Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves
• Impact of nuclear masses on r-process nucleosynthesis: bulk properties versus shell effects
• Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy
• The apparent and cosmic rates of short gamma-ray bursts
• Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
• Charged black holes in Eddington-inspired Born-Infeld gravity: An in-depth analysis of the structure of spacetime geometry
• labrador: A domain-optimized machine-learning tool for gravitational wave inference
• A Novel Search Technique for Low-Frequency Periodic Gravitational Waves
• Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
• On the hosts of neutron star mergers in the nearby Universe
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring
• Density functional approach to quark matter with confinement and color superconductivity
• Modeling the Galactic Neutron Star Population for Use in Continuous Gravitational Wave Searches
• $f$-mode Oscillations for Hyperons and H-dibaryons in Neutron Stars
• Identification of new gold lines in the 350 to 1000 nm spectral region using laser produced plasmas
• Effectiveness of Stacks in the Stacked Hilbert-Huang Transform
• Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries
• A viable relativistic scalar theory of gravitation
• The thermal index of neutron-star matter in the virial approximation
• Single-Pulse Gamma-Ray Bursts have Prevalent Hard-to-Soft Spectral Evolution
• Aspects of astrophysical particle production and beyond the Standard Model phenomenology
• New trends in the general relativistic Poynting-Robertson effect modeling
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Predictions on observing hot holographic quark star with gravitational waves
• Extreme Transients in Gamma Rays
• Building A Field: The Future of Astronomy with Gravitational Waves, A State of The Profession Consideration for Astro2020
• Unexpected Symmetries of Kerr Black Hole Scattering
• Convective stability analysis of massive neutron stars formed in binary mergers
• Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes
• Updated estimates of post-merger gravitational wave energy released in GW170817 and the maximum neutron star mass
• Gravitational-wave standard sirens and application in cosmology
• Effect of primary scalar hair on black hole's strong lensing in Beyond Horndeski Gravity
• Scalar-scalar-tensor interaction in DHOST theories
• Impact of Higher-order Tidal Corrections on the Measurement Accuracy of Neutron Star Tidal Deformability
• Exploring the Link between Fast Radio Burst and Binary Neutron Star Origins with Spaceborne Gravitational Wave Observations
• Terrestrial Laser Interferometers
• The Origins of Neutron-capture Elements In Globular Cluster M22
• Analogue Black Holes in Reactive Molecules
• Search for Deeply Bound Kaonic Nuclear States with AMADEUS
• Nonradial oscillations of realistic anisotropic neutron stars: Axial modes
• Frozen-In Gravitational Fields
• Primordial gravitational waves: Model effects on time evolution and spectrum
• Gravitational wave astronomy: astrophysical and cosmological inferences
• Chandra X-ray Observations of the Neutron Star Merger GW170817: Thermal X-Ray Emission From a Kilonova Remnant?
• Perturbations and stability conditions of k-essence and kinetic gravity braiding models in two-field measure theory
• Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study
• Slowly rotating condensate dark stars beyond the mean-field approximation
• Strongly Interacting Dark Matter admixed Neutron Stars
• Universality of dual mass-scaled fundamental modes in two-fluid neutron stars with mirror dark matter
• Constraining Scalar Charge in Neutron Stars through Gravitational Wave Signals from NSBH Mergers
• Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
• Stochastic gravitational wave background from the collisions of dark matter halos
• The $g$-mode frequencies in cold neutron stars and nuclear saturation parameters
• Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes
• Apparatus to Measure Optical Scatter of Coatings Versus Annealing Temperature
• Impact and detectability of spin-tidal couplings in neutron star inspirals
• Testing f(R) gravity using gravitational-wave signals from binary mergers
• Synchrotron self-Compton Reverse Shock in Energy-Injection and Radiative Scenarios