Science Case for the Einstein Telescope

Abstract

The Einstein Telescope (ET), a proposed European ground-based gravitational-wave detector of third-generation, is an evolution of second-generation detectors such as Advanced LIGO, Advanced Virgo, and KAGRA which could be operating in the mid 2030s. ET will explore the universe with gravitational waves up to cosmological distances. We discuss its main scientific objectives and its potential for discoveries in astrophysics, cosmology and fundamental physics.

51 pages, 14 figures; v3: references added, various improvements. v4: minor changes. Version published in JCAP

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• Planck 2018 results. VI. Cosmological parameters
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• Maximum elastic deformations of relativistic stars
• Cosmology with the lights off: Standard sirens in the Einstein Telescope era
• The gravitational-wave luminosity distance in modified gravity theories
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• Cosmological phase transitions: from perturbative particle physics to gravitational waves
• Gravitational waves from a universe filled with primordial black holes
• Massively parallel Bayesian inference for transient gravitational-wave astronomy
• Observational Evidence for Primordial Black Holes: A Positivist Perspective
• Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
• Primordial Black Holes Confront LIGO/Virgo data: Current situation
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
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• Baryogenesis from the weak scale to the grand unification scale
• Conservative Dynamics of Binary Systems at Fourth Post-Minkowskian Order in the Large-eccentricity Expansion
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• Dynamical Friction in Gravitational Atoms
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• The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes
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• Black Holes in $f(T,B)$ Gravity: Exact and Perturbed Solutions
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• Measuring the net circular polarization of the stochastic gravitational wave background with interferometers
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• The Imprint of Relativistic Particles on the Anisotropies of the Stochastic Gravitational-Wave Background
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• Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects
• Gravity Gradient Noise from Asteroids
• Globular cluster formation histories, masses and radii inferred from gravitational waves
• New universal property of cosmological gravitational wave anisotropies
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• Resonant Shattering Flares in Black Hole-Neutron Star and Binary Neutron Star Mergers
• Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
• Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Toward the primordial black hole formation threshold in a time-dependent equation-of-state background
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• Self-force framework for transition-to-plunge waveforms
• Lensing constraints on ultradense dark matter halos
• Upper Bound on Thermal Gravitational Wave Backgrounds from Hidden Sectors
• High Energy Neutrinos from Choked Gamma-Ray Bursts in AGN Accretion Disks
• Modified gravitational wave propagation with higher modes and its degeneracies with lensing
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• Learning how to surf: Reconstructing the propagation and origin of gravitational waves with Gaussian Processes
• Pre-merger alert to detect the very-high-energy prompt emission from binary neutron-star mergers: Einstein Telescope and Cherenkov Telescope Array synergy
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• Self-consistent adiabatic inspiral and transition motion
• Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods
• Dense Matter in Neutron Stars with eXTP
• Sharp turns in axion monodromy: primordial black holes and gravitational waves
• Inference of the neutron star equation of state from cosmological distances
• Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
• Observation of eccentric binary black hole mergers with second and third generation gravitational wave detector networks
• The Dipole of the Astrophysical Gravitational-Wave Background
• Methods and prospects for gravitational wave searches targeting ultralight vector boson clouds around known black holes
• Eccentric Binary Neutron Star Search Prospects for Cosmic Explorer
• Lensing of gravitational waves: universal signatures in the beating pattern
• Exploring compact binary populations with the Einstein Telescope
• Gravitational Lensing of Gravitational Waves: Probability of Microlensing in Galaxy-Scale Lens Population
• Measuring tidal effects with the Einstein Telescope: A design study
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Constraining three-nucleon forces with multimessenger data
• Induced Gravitational Waves probing Primordial Black Hole Dark Matter with Memory Burden
• Forming merging double compact objects with stable mass transfer
• New Gravitational Wave Discoveries Enabled by Machine Learning
• Bayesian parameter estimation on boson-star binary signals with a coherent inspiral template and spin-dependent quadrupolar corrections
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Constraints on $f(Q)$ logarithmic model using gravitational wave standard sirens
• Study of the Intermediate Mass Ratio Black Hole Binary Merger up to 1000:1 with Numerical Relativity
• Evidence of extended emission in GRB 181123B and other high-redshift short GRBs
• Non-Markovian open quantum system approach to the early universe: I. Damping of gravitational waves by matter
• Searching for General Binary Inspirals with Gravitational Waves
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• Gravitational waves from accretion-induced descalarization in massive scalar-tensor theory
• A Gravitational Wave Detector for Post Merger Neutron Stars: Beyond the Quantum Loss Limit of Michelson Fabry Perot Interferometer
• Searching for High Frequency Gravitational Waves with Phonons
• The non-linear dynamics of axion inflation: a detailed lattice study
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Utilizing the null stream of the Einstein Telescope
• Impact of a Midband Gravitational Wave Experiment On Detectability of Cosmological Stochastic Gravitational Wave Backgrounds
• Future prospects on testing extensions to $\Lambda$CDM through the weak lensing of gravitational waves
• Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes
• Spinning particles near Kerr black holes: Orbits and gravitational-wave fluxes through the Hamilton-Jacobi formalism
• Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories
• Scalar induced gravitational waves in modified teleparallel gravity theories
• Merger-Ringdown Consistency: A New Test of Strong Gravity using Deep Learning
• Gravitational-wave cosmological distances in scalar-tensor theories of gravity
• Clustering of Gravitational Wave and Supernovae events: a multitracer analysis in Luminosity Distance Space
• Tidal Love numbers and approximate universal relations for fermion soliton stars
• 50 Years of Horndeski Gravity: Past, Present and Future
• Small-scale Tests of Inflation
• Probing dipole radiation from binary neutron stars with ground-based laser-interferometer and atom-interferometer gravitational-wave observatories
• Analyzing clustering of astrophysical gravitational-wave sources: Luminosity-distance space distortions
• Vanishing of Quadratic Love Numbers of Schwarzschild Black Holes
• Hunting WIMPs with LISA: Correlating dark matter and gravitational wave signals
• Gravitational-wave dark siren cosmology systematics from galaxy weighting
• Modified gravitational wave propagation and the binary neutron star mass function
• Asteroseismology using quadrupolar f-modes revisited: breaking of universal relationships in the slow hadron-quark conversion scenario
• Gravitational Waves from Black-Hole Encounters: Prospects for Ground- and Galaxy-Based Observatories
• The KAGRA underground environment and lessons for the Einstein Telescope
• Source anisotropies and pulsar timing arrays
• Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches
• The effect of multiple features on the power spectrum in two-field inflation
• Searching For Stochastic Gravitational Waves Below a Nanohertz
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Orbital eccentricity in general relativity from catastrophe theory
• Magnetogenesis with gravitational waves and primordial black hole dark matter
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Detection and estimation of the cosmic dipole with the Einstein Telescope and Cosmic Explorer
• Observational prospects of self-interacting scalar superradiance with next-generation gravitational-wave detectors
• Constraining mass, radius and tidal deformability of compact stars with axial wI modes: new universal relations including slow stable hybrid stars
• PyROQ: a Python-based Reduced Order Quadrature Building Code for Fast Gravitational Wave Inference
• The observed number counts in luminosity distance space
• Frequency- and polarization-dependent lensing of gravitational waves in strong gravitational fields
• Testing the nature of dark compact objects with gravitational waves
• Prospects for detecting transient quasi-monochromatic gravitational waves from glitching pulsars with current and future detectors
• Rapidly rotating neutron stars: Universal relations and EOS inference
• Nonlocal-in-time effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Hot neutron stars and their equation of state
• Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds
• Implication of Pulsar Timing Array Experiments on Cosmological Gravitational Wave Detection
• Microscopic nuclear equation of state at finite temperature and stellar stability
• The fate of twin stars on the unstable branch: implications for the formation of twin stars
• Extreme mass ratio inspirals in rotating dark matter spikes
• Testing the Speed of Gravity with Black Hole Ringdown
• Gravitational waves from burdened primordial black holes dark matter
• Accretion-modified stellar-mass black hole distribution and milli-Hz gravitational wave backgrounds from galaxy centre
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Self-Interacting Gravitational Atoms in the Strong-Gravity Regime
• 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
• A Robust Test of the Existence of Primordial Black Holes in Galactic Dark Matter Halos
• Constraining $\Lambda$CDM cosmological parameters with Einstein Telescope mock data
• Dipolar tidal effects in gravitational waves from scalarized black hole binary inspirals in quadratic gravity
• New search pipeline for gravitational waves with higher-order modes using mode-by-mode filtering
• A lower limit for Newtonian-noise models of the Einstein Telescope
• Constraining Horndeski theory with gravitational waves from coalescing binaries
• 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
• 2.5PN accurate waveform information for generic-planar-orbit binaries in effective one-body models
• Resolving phase transition properties of dense matter through tidal-excited g-mode from inspiralling neutron stars
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• The potential role of binary neutron star merger afterglows in multimessenger cosmology
• Gravitational-Wave Searches for Cosmic String Cusps in Einstein Telescope Data using Deep Learning
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• Parity violation in gravitational waves and observational bounds from third-generation detectors
• Redshift evolution of primordial black hole merger rate
• Detectability of continuous gravitational waves from isolated neutron stars in the Milky Way: the population synthesis approach
• Primordial Black Hole Formation in Non-Standard Post-Inflationary Epochs
• Forecasts on interacting dark energy with standard sirens
• Astrometric Gravitational-Wave Detection via Stellar Interferometry
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Constraining extended cosmologies with GW$\times$LSS cross-correlations
• LADDER: Revisiting the Cosmic Distance Ladder with Deep Learning Approaches and Exploring its Applications
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Formation of Merging Stellar-Mass Black Hole Binaries by Gravitational Wave Emission in Active Galactic Nucleus Disks
• Effects of orbital precession on hyperbolic encounters
• Multi-messenger Gravitational Lensing
• Performance-Portable Binary Neutron Star Mergers with AthenaK
• Photon Counting Interferometry to Detect Geontropic Space-Time Fluctuations with GQuEST
• I-Love-$⟨c_s^2⟩$: Approximately universal relations for the average neutron star stiffness
• Glitching pulsars as gravitational wave sources
• Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
• On the primordial black hole formation in hybrid inflation
• Using Pulsar Parameter Drifts to Detect Sub-Nanohertz Gravitational Waves
• Testing gravity with gravitational wave friction and gravitational slip
• Searching for Dark Clumps with Gravitational-Wave Detectors
• Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
• Signal Space in the Triangular Network of Einstein Telescope
• 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
• Tomography of flavoured leptogenesis with primordial blue gravitational waves
• Constraints on charged black holes from merger-ringdown signals in GWTC-3 and prospects for the Einstein Telescope
• Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
• Primordial Stochastic Gravitational Wave Background Anisotropies: in-in Formalization and Applications
• Prospects of constraining $f(T)$ gravity with the third-generation gravitational-wave detectors
• Linear vs. nonlinear modeling of black hole ringdowns
• Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
• Conditions for direct black hole seed collapse near a radio-loud quasar 1 Gyr after the Big Bang
• Hierarchical approach to matched filtering using a reduced basis
• SLICK: Strong Lensing Identification of Candidates Kindred in gravitational wave data
• Detection possibility of continuous gravitational waves from rotating magnetized neutron stars
• Constraining changes in the merger history of (P)BH binaries with the stochastic gravitational wave background
• Adaptive mesh refinement in binary black holes simulations
• Quasinormal modes of black holes encircled by a gravitating thin disk
• Frequency-dependent squeezing for gravitational-wave detection through quantum teleportation
• Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
• Identifying modified theories of gravity using binary black-hole ringdowns
• Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Prospects for Direct Detection of Black Hole Formation in Neutron Star Mergers with Next-Generation Gravitational-Wave Detectors
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• The Electro-Weak Phase Transition at Colliders: Discovery Post-Mortem
• Enhancing interferometer sensitivity without sacrificing bandwidth and stability: beyond single-mode and resolved-sideband approximation
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Polytropic fits of modern and unified equations of state
• Mechanisms for producing Primordial Black Holes from Inflationary Models Beyond Fine-Tuning
• Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability
• Precision Ephemerides for Gravitational-wave Searches -- IV: Corrected and refined ephemeris for Scorpius X-1
• Gravitational-wave background in bouncing models from semi-classical, quantum and string gravity
• Compact Binaries through a Lens: Silent vs. Detectable Microlensing for the LIGO-Virgo-KAGRA Gravitational Wave Observatories
• Role of spatial curvature in the primordial gravitational wave power spectrum
• A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens
• The luminosity functions of kilonovae from binary neutron star mergers under different equation of states
• No slip gravity in light of LISA standard sirens
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Sensitivity of third-generation interferometers to extra polarizations in the Stochastic Gravitational Wave Background
• On the Merger Rate of Primordial Black Holes in Cosmic Voids
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Stochastic gravitational wave background: birth from string-wall death
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Cosmological Tests of Gravity: A Future Perspective
• On the integrability of extended test body dynamics around black holes
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Validating Prior-informed Fisher-matrix Analyses against GWTC Data
• Boltzmann equations for astrophysical Stochastic Gravitational Wave Backgrounds scattering off of massive objects
• Implications for Cosmic Domain Walls from LIGO-Virgo First Three Observing Runs
• Strong-lensing cosmography using third-generation gravitational-wave detectors
• Numerical convergence of model Cauchy-characteristic extraction and matching
• Premerger phenomena in neutron-star binary coalescences
• Matched filtering for gravitational wave detection without template bank driven by deep learning template prediction model bank
• Emulators for Scarce and Noisy Data: Application to Auxiliary-Field Diffusion Monte Carlo for Neutron Matter
• Effects of mixing and annealing on the optical and mechanical properties of TiO${}_2$:Ta${}_2$O${}_5$ amorphous coatings
• Detection of Einstein Telescope gravitational wave signals from binary black holes using deep learning
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Universality in quasinormal modes of neutron stars with quark-hadron crossover
• The rise of the primordial tensor spectrum from an early scalar-tensor epoch
• Gravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors
• How many extra-Galactic stellar-mass binary black holes will be detected by space gravitational-wave interferometers?
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
• Real modes and null memory contributions in effective-one-body models
• Detectability of stochastic gravitational wave background from weakly hyperbolic encounters
• Leptogenesis, Dark Matter and Gravitational Waves from Discrete Symmetry Breaking
• Nondegenerate internal squeezing: an all-optical, loss-resistant quantum technique for gravitational-wave detection
• Gravitational lensing of gravitational waves: prospects for probing intermediate-mass black holes in galaxy lenses with global minima image
• Quasi-universal relations in the context of future neutron star detections
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Early warning of precessing compact binary merger with third-generation gravitational-wave detectors
• Feasibility study of beam-expanding telescopes in the interferometer arms for the Einstein Telescope
• Stochastic waveform estimation at the fundamental quantum limit
• Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities
• The effect of screening mechanisms on black hole binary inspiral waveforms
• Primary hairs may create echoes
• The imprint of superradiance on hierarchical black hole mergers
• Cosmological Consequences of Domain Walls Biased by Quantum Gravity
• Quantifying Systematic Biases in Black Hole Spectroscopy
• Exploring Fermionic Dark Matter Admixed Neutron Stars in the Light of Astrophysical Observations
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Signature of hadron-quark crossover in binary-neutron-star mergers
• Cosmic Cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure
• First Search for Ultralight Dark Matter Using a Magnetically Levitated Particle
• On the response of the Einstein Telescope to Doppler anisotropies
• Perturbative and non-linear analyses of gravitational turbulence in spacetimes with stable light rings
• Scalable data-analysis framework for long-duration gravitational waves from compact binaries using short Fourier transforms
• Observational Signatures of Massive Black Hole Progenitor Pathways: Could Leo I a Smoking Gun?
• Study on the detectability of gravitational radiation from single-binary encounters between black holes in nuclear star cluster: the case of hyperbolic flybys
• Gravitational-wave event rates as a new probe for dark matter microphysics
• Constraining the ellipticity of millisecond pulsars with observed spin-down rates
• Whispers from the quantum core: the ringdown of semiclassical stars
• Outliers in the LIGO Black Hole Mass Function from Coagulation in Dense Clusters
• The Effect of Multiple Cooling Channels on the Formation of Dark Compact Objects
• Scalar emission from neutron star-black hole binaries in scalar-tensor theories with kinetic screening
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Covariant formulation of refracted gravity
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• Inferring Interference: Identifying a Perturbing Tertiary with Eccentric Gravitational Wave Burst Timing
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• Probing dark-matter effects with gravitational waves using the parameterized post-Einsteinian framework
• Prospects of Probing Dark Matter Condensates with Gravitational Waves
• Formation and fate of low metallicity stars in IllustrisTNG50
• GPU-accelerated LISA parameter estimation with full time domain response
• Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
• Detectability of strongly lensed gravitational waves using model-independent image parameters
• Probing loop quantum effects through solar system experiments: observational signatures and parameter constraints
• Testing the robustness of simulation-based gravitational-wave population inference
• Impact of overlapping signals on parameterized post-Newtonian coefficients in tests of gravity
• Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach
• Worldtube excision method for intermediate-mass-ratio inspirals: scalar-field model in 3+1 dimensions
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Probing Interacting Dark Sector with the next generation of gravitational-wave detectors
• Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G
• Multiple peaks in gravitational waves induced from primordial curvature perturbations with non-Gaussianity
• Maximal GW amplitude from bubble collisions in supercooled phase transitions
• Solar System-scale interferometry on fast radio bursts could measure cosmic distances with sub-percent precision
• Ringdowns for black holes with scalar hair: the large mass case
• Higher-order tails and RG flows due to scattering of gravitational radiation from binary inspirals
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• A model-independent tripartite test of cosmic distance relations
• Systematic biases from ignoring environmental tidal effects in gravitational wave observations
• Scalar induced gravitational waves review
• A vertical inertial sensor with interferometric readout
• Modern Cosmology, an Amuse-Gueule
• Applications of the close-limit approximation: horizonless compact objects and scalar fields
• Effects of Galaxy Cluster Structure on Lensed Gravitational Waves
• The effect of quantum decoherence on inflationary gravitational waves
• Deep learning to detect gravitational waves from binary close encounters: Fast parameter estimation using normalizing flows
• Fundamental Physics and Cosmology with TianQin
• Inverse problem of analog gravity systems
• Identifying thermal effects in neutron star merger remnants with model-agnostic waveform reconstructions and third-generation detectors
• Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
• Evaporating black holes: constraints on anomalous emission mechanisms
• On the origin of quasinormal modes in semi-open systems
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• HERMES: Gamma Ray Burst and Gravitational Wave counterpart hunter
• The curvature dependence of gravitational-wave tests of General Relativity
• Binary dynamics to second post-Newtonian order in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity from effective field theory
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• Precessing Binary Black Holes as Better Dark Sirens
• Revealing Dark Matter's Role in Neutron Stars Anisotropy: A Bayesian Approach Using Multi-messenger Observations
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• Impact of gravitational waveform model systematics on the measurement of the Hubble constant
• Ultra-compact binary pulsars as continuous dual-line gravitational wave sources
• Prospects for detecting neutron star-white dwarf mergers with decihertz gravitational-wave observatories
• Transition-to-plunge self-force waveforms with a spinning primary
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Gravitational Waves from Metastable Cosmic Strings in Supersymmetric New Inflation Model
• Solar Diffraction of LIGO-Band Gravitational Waves
• Blind source separation in 3rd generation gravitational-wave detectors
• Observational prospects for phase transitions at LISA: Fisher matrix analysis
• Anisotropies of cosmological gravitational wave backgrounds in non-flat spacetime
• Forecasting the population properties of merging black holes
• Future targets for light gauge bosons from cosmic strings
• Gravitational waves from cosmic strings in Froggatt-Nielsen flavour models
• Probing axion-like particles with multimessenger observations of neutron star mergers
• New Source for QCD Axion Dark Matter Production: Curvature Induced
• The Formation of Electron-capture Supernovae: A Review
• Magnification and evolution bias of transient sources: GWs and SNIa
• Impact of the cosmic neutrino background on black hole superradiance
• Inferring three-nucleon couplings from multi-messenger neutron-star observations
• Gravitational tests of electroweak relaxation
• Likelihood for a Network of Gravitational-Wave Detectors with Correlated Noise
• Amplified Squeezed States: Analyzing Loss and Phase Noise
• High-energy neutrino signatures from pulsar remnants of binary neutron-star mergers: coincident detection prospects with gravitational waves
• Scalar-Induced Gravitational Waves in a $\Lambda$CDM Cosmology
• Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors
• Enhanced tensor non-Gaussianities in presence of a source
• Scalar-Induced Gravitational Waves in Modified Gravity
• The First Model-Independent Chromatic Microlensing Search: No Evidence in the Gravitational Wave Catalog of LIGO-Virgo-KAGRA
• A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
• Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
• Prospects for Time-Domain and Multi-Messenger Science with eXTP
• Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2
• Gravitational waves from nonradial oscillations of stochastically accreting neutron stars
• Impact of signal clusters in wide-band searches for continuous gravitational waves
• Relevance of Precession for Tests of the Black Hole No Hair Theorems
• Purely metric Horndeski theories and spontaneous curvaturization of black holes
• Boundary conditions for stationary black holes ; Application to Kerr, Martinez-Troncoso-Zanelli and hairy black holes
• Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer
• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• Covariant approach to relativistic large-eddy simulations: Lagrangian filtering
• Scalar Quasinormal Modes of Rotating Regular Black Holes
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Neutron displacement noise-free interferometer for gravitational-wave detection
• Multi-messenger observations in the Einstein Telescope era: binary neutron star and black hole - neutron star mergers
• Breaking parity: the case of the trispectrum from chiral scalar-tensor theories of gravity
• Crescendo Beyond the Horizon: More Gravitational Waves from Domain Walls Bounded by Inflated Cosmic Strings
• Forecast Analysis of Astrophysical Stochastic Gravitational Wave Background beyond general relativity: A Case Study on Brans-Dicke Gravity
• Unraveling the CMB lack-of-correlation anomaly with the cosmological gravitational wave background
• Gravitational waves from quasielliptic compact binaries in scalar-tensor theory to one-and-a-half post-Newtonian order
• Using Gravitational Wave Signals to Disentangle Early Matter Dominated Epochs
• Impact of weak lensing on bright standard siren analyses
• Quantum gravity and gravitational-wave astronomy
• The impact of waveform systematics and Gaussian noise on the interpretation of GW231123
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• CLAP for modified gravity: scalar instabilities in binary black hole spacetimes
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• Next step in gravity and cosmology: fundamental theory or data-driven models?
• Mass octupole and current quadrupole corrections to gravitational wave emission from close hyperbolic encounters
• Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT
• X- and Gamma-ray astrophysics in the era of Multi-messenger astronomy
• Multi-messenger FIMP
• Fast Radio Bursts as crustal dynamical events induced by magnetic field evolution in young magnetars
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
• Theory-agnostic searches for non-gravitational modes in black hole ringdown
• New model of spontaneous scalarization of black holes induced by curvature and matter
• Gravitational Wave Propagation and Polarizations in the Teleparallel analog of Horndeski Gravity
• Effects of inner crusts on $g$-mode oscillations in neutron stars
• The first law of binary black hole scattering
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Probing eccentric higher-order modes through an effective chirp mass model
• Spectral instability of horizonless compact objects within astrophysical environments
• Advancing the Effective-One-Body Framework in the Test-Mass Limit
• Gravitational wave background from primordial black holes in globular clusters
• Love-C relations for elastic hybrid stars
• ROXAS: a new pseudospectral non-linear code for general relativistic oscillations of fast rotating isolated neutron stars
• How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
• Compact Binary Coalescence Gravitational Wave Signals Counting and Separation
• Gravitational wave lensing: probing Fuzzy Dark Matter with LISA
• Constraining primordial tensor features with the anisotropies of the Cosmic Microwave Background
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• Earth rotation and time-domain reconstruction of polarization states for continuous gravitational waves from a known pulsar
• Physics-inspired spatiotemporal-graph AI ensemble for the detection of higher order wave mode signals of spinning binary black hole mergers
• The impact of local noise recorded at the ET candidate sites on the signal to noise ratio of CBC gravitational wave signals for the ET triangle configuration
• Propagation and lensing of gravitational waves in Palatini $f(\hat{R})$ gravity
• Non-analytic behavior of the relativistic r-modes in slowly rotating neutron stars
• Inverse bubbles from broken supersymmetry
• Reconstructing the LISA massive black hole binary population via iterative kernel density estimation
• Frequency-Domain Distribution of Astrophysical Gravitational-Wave Backgrounds
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations
• Assessing the similarity of continuous gravitational-wave signals to narrow instrumental artifacts
• Cosmic Strings as Dynamical Dark Energy: Novel Constraints
• The population of NuSTAR Black Hole X-ray Binaries
• Search for sub-solar mass binaries with Einstein Telescope and Cosmic Explorer
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• Potential impact of noise correlation in next-generation gravitational wave detectors
• Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone
• Lessons on early structure formation from a mature galaxy cluster observed at cosmic noon
• Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity
• Reconstructing the star formation rate for compact binary populations with the Einstein telescope
• DeepSSM: an emulator of gravitational wave spectra from sound waves during cosmological first-order phase transitions
• Unstable modes of hypermassive compact stars driven by viscosity and gravitational radiation
• Gravitational wave signals from long lasting binary-single black hole encounters
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
• Atmospheric Newtonian noise modeling for third-generation gravitational wave detectors
• Probing the Growth of Massive Black Holes with Black Hole-Host Galaxy Spin Correlations
• Nonlinear Ringdowns as Sources and Detectors of Quantum Gravitational Waves
• Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes
• Measuring the primordial gravitational waves from cosmic microwave background and stochastic gravitational wave background observations
• Measuring the speed of gravity and the cosmic expansion with time delays between gravity and light from binary neutron stars
• Black hole spectroscopy of collapsing and merging neutron stars
• Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
• Gravitational Signatures of Axion Dark Matter via Parity-Violating Interactions
• A hydrodynamical description of gravitational waves
• Detecting the heterodyning of gravitational waves
• Kilonova-Targeting Lightcurve Classification for Wide Field Survey Telescope
• Log-periodic gravitational-wave background beyond Einstein gravity
• Merging Black Holes: Assessing the Performance of Two Analytic Gravitational Waves Models
• Gravitational Wave Emission from Close-in Strange Quark Planets Around Strange Stars with Magnetic Interactions
• Eccentric Pairs: Analytic Gravitational Waves from Binary Black Holes in Elliptic Orbits
• Impact of gravitational lensing on black hole mass function inference with third-generation gravitational wave detectors
• The THESEUS space mission: science goals, requirements and mission concept
• Secular dipole-dipole stability of magnetic binaries
• Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
• Beyond the Long Wavelength Approximation: Next-generation Gravitational-Wave Detectors and Frequency-dependent Antenna Patterns
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• Gravitational waves from primordial black hole dominance: The effect of inflaton decay rate
• Multi-Messenger Astrophysics with THESEUS in the 2030s
• Post-inflationary Leptogenesis and Dark Matter production: Metric versus Palatini formalism
• Forecast cosmological constraints from the number counts of Gravitational Waves events
• Hierarchical searches for subsolar-mass binaries and the third-generation gravitational wave detector era
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Probing black holes via quasinormal modes in a dark energy-induced dark matter
• A post-Newtonian approach to neutron star oscillations
• Signatures of asymmetry: Gravitational wave memory and the parity violation
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• A potential third-generation gravitational-wave detector based on autocorrelative weak-value amplification
• Constraining the environment of compact binary mergers with self-lensing signatures
• A New Source of Phase Transition Gravitational Waves: Heavy Particle Braking Across Bubble Walls
• Testing gravity with the latent heat of neutron star matter
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• Fully consistent rotating black holes in the cubic Galileon theory
• Cosmological forecasts from the combination of Stage-IV photometric galaxy surveys and the magnification from forthcoming GW observatories
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Quantum gravity phenomenology from the perspective of quantum general relativity and quadratic gravity
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• A density-responsive scalar-field framework for singularity regularization and dynamical dark energy
• A weakly-modeled search for compact binary coalescences in Einstein Telescope
• Merger History of Clustered Primordial Black Holes
• Effect of spin in binary neutron star mergers
• Scalar-induced gravitational waves including isocurvature perturbations with lattice simulations
• Freeze-in gravitational waves and dark matter in warm inflation
• On-shell approach to scalar hair in spinning binaries
• Tests of general relativity at the fourth post-Newtonian order
• One-stop strategy to search for long-duration gravitational-wave signals
• Hybrid inflation and gravitational waves from accidentally light scalars
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• Co-interacting dark matter and conformally coupled light scalars
• The Repulsive Effect of Covariant Effective Quantum Gravity
• Gravitational waves from a first-order phase transition of the inflaton
• Relative calibration of the LIGO and Virgo detectors using astrophysical events from their third observing run
• Rigorous analytic solution to the gravitational-wave overlapping event rates
• Astrophysical constraints on neutron star $f$-modes with a nonparametric equation of state representation
• Nyquist-resolving gravitational waves via orbital frequency-based refinement
• Neutrinos in colliding neutron stars and black holes
• Equations of motion for compact binary systems in general relativity: Do they depend on the bodies' internal structure at the third post-Newtonian order?
• The landscape of massive black-hole spectroscopy with LISA and Einstein Telescope
• Resonant amplification of multimessenger emission in rotating stellar core collapse
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• The Luminosity of the Darkness: Schechter function in dark sirens
• Supersymmetric Horizons at the Edge of Effective Field Theory
• Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• Kilohertz Gravitational Waves from Binary Neutron Star Mergers: Full Spectrum Analyses and High-density Constraints on Neutron Star Matter
• Quantum Machine Learning for Identifying Transient Events in X-ray Light Curves
• Classification of radial Kerr geodesic motion
• Baryogenesis via relativistic bubble expansion
• Absorption spectroscopy of quantum black holes with gravitational waves
• Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
• Primordial black holes versus their impersonators at gravitational wave observatories
• Eikonal gravitational-wave lensing in Einstein-aether theory
• Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates
• Compact binary system dynamics at the second post-Newtonian order: analytical formula of the coordinate time for eccentric and circular orbits
• Stochastic gravitational wave from graviton bremsstrahlung in inflaton decay into massive spin 3/2 particles
• Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors
• Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation
• Gravitational waves from primordial black holes passing by neutron stars: observational prospects for the Galactic center
• Pushing spectral siren cosmology into the third-generation era: a blinded mock data challenge
• Radial Oscillations of Viscous Stars
• Large-Scale Dynamos Driven by Shear-Flow-Induced Jets
• Adaptive Modeling of Correlated Noise in Space-Based Gravitational Wave Detectors
• Continuous gravitational waves from thermal mountains on accreting neutron stars: effect of the nuclear pasta phase
• Tidal Love numbers of a nonexotic compact object with a thin shell
• Eccentricity evolution of spinning binaries and its dependence on the equation of state of the components
• Constraining scotogenic dark matter and primordial black holes using gravitational waves
• Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
• Beyond general relativity: gravitational waves in non-minimally coupled theories
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• Impact of correlated seismic and correlated Newtonian noise on the Einstein Telescope
• Terrestrial Laser Interferometers
• Circularly polarized gravitational waves from parity-violating scalar-tensor theory
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
• Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
• Rising Tides: Analytic Modeling of Tidal Effects in Binary Neutron Star Mergers
• Probing cosmology with bright sirens from the CosmoDC2_BCO LSST synthetic catalog
• Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433
• Direct N-body simulations of rotating and extremely massive Population III star clusters
• GEMINI: The First Underground Testbed for Seismic Isolation and Interplatform Control in Next-Generation Gravitational-Wave Detectors
• Smoking Gun Signatures of Quasilocal Probability in Black Hole Ringdowns
• Primordial Black Holes: A Review of Formation and Evolution
• Tidal Love numbers and the dynamical instability of AdS bubbles
• Efficient Evaluation of Gravitational Lensing Amplification Factors: A Deep Learning Framework
• Gravitational-wave standard sirens and application in cosmology
• Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors
• Testing f(R) gravity using gravitational-wave signals from binary mergers
• Impact and detectability of spin-tidal couplings in neutron star inspirals
• Multi-messenger lensing time delay as a probe of the graviton mass
• $f$-mode Oscillations for Hyperons and H-dibaryons in Neutron Stars
• Effects of local cosmic inhomogeneities on the gravitational wave event rate
• GWCloud: a searchable repository for the creation and curation of gravitational-wave inference results
• Propagation and emission of gravitational waves in the weak-field limit within the Palatini formalism
• Baryogenesis via relativistic bubble walls
• Detector induced anisotropies on the angular distribution of gravitational wave sources and opportunities of constraining horizon scale anisotropies
• Gamma-radiation sky maps from compact binaries
• Multi-scale optimal control for Einstein Telescope active seismic isolation
• Production of relic gravitational waves and the baryon asymmetry of the universe by random hypermagnetic fields
• Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
• $e^{+}{e}^{-}$ annihilation on the stochastic background of primordial gravitational waves with BKP18
• Precision Joint Constraints on Cosmology and Gravity Using Strongly Lensed Gravitational Wave Populations
• Parameter inference of millilensed gravitational waves using neural spline flows
• Hamiltonian normal forms for the post-Newtonian binary problem
• Source Confusion of Massive Black Hole Binaries for the Taiji Mission
• Gravitational wave background from mergers of large primordial black holes
• $\kappa$-General-Relativity II: An Astrophysical Observable from a 2-Body system
• Signatures of Primordial Gravitational Waves on the Large-Scale Structure of the Universe
• Mergers as a Probe of Particle Dark Matter
• 1PN effective binary Lagrangian for the gravity-Kalb-Ramond sector in the conservative regime
• Probing modified gravitational wave propagation with strongly lensed coalescing binaries
• Differentiating between sharp and smoother phase transitions in neutron stars
• Mutated hilltop inflation in light of Planck/ACT observations
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• Exploiting Newton-factorized, 2PN-accurate, waveform multipoles in effective-one-body models for spin-aligned noncircularized binaries
• A Faster Growth of Perturbations in an Early Matter Dominated Epoch: Primordial Black Holes and Gravitational Waves
• Dynamical double black holes and their host cluster properties
• Correlating Gravitational Wave and Gamma-ray Signals from Primordial Black Holes
• Bridging inflation and reheating: chiral gravitational waves from aHz to GHz
• Constraining the Nuclear Equation of State from Rotating Neutron Stars
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars
• Trails of clouds in binary black holes
• On the logarithmic Love number of black holes beyond general relativity
• Probing Bose-enhanced Inflaton Decay with Gravitational Waves
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands
• Detectability of the Phase Transition Gravitational Waves in the DFSZ axion Model
• Sco X-1 as a continuous gravitational waves source: modelling the secular evolution using MESA
• Constraining Hamiltonians from chiral effective field theory with neutron-star data
• Extremal Love: tidal/electromagnetic deformability, logarithmic running and the weak gravity conjecture