Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

Abstract

The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.

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• Testing clockwork axion with gravitational waves
• Constraints on the ultralight scalar boson from Advanced LIGO and Advanced Virgo's first three observing runs using the stochastic gravitational-wave background
• Landscape of stellar-mass black-hole spectroscopy with third-generation gravitational-wave detectors
• Astrophysics with core-collapse supernova gravitational wave signals in the next generation of gravitational wave detectors
• Tidal deformations of hybrid stars with sharp phase transitions and elastic crusts
• Excitation of f-modes during mergers of spinning binary neutron star
• Searching for hypermassive neutron stars with short gamma-ray bursts
• Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers
• Reduced-order surrogate models for scalar-tensor gravity in the strong field and applications to binary pulsars and GW170817
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• A 6D interferometric inertial isolation system
• Cosmography with next-generation gravitational wave detectors
• Towards distinguishing Dirac from Majorana neutrino mass with gravitational waves
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
• Regression methods in waveform modeling: a comparative study
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Axion dark matter search using arm cavity transmitted beams of gravitational wave detectors
• Inspiralling eccentric binary neutron stars: orbital motion and tidal resonance
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• How loud are echoes from exotic compact objects?
• Leveraging gravitational-wave memory to distinguish neutron star--black hole binaries from black hole binaries
• Probing Crust Meltdown in Inspiraling Binary Neutron Stars
• Core collapse in massive scalar-tensor gravity
• Laser Frequency Noise in Next Generation Gravitational-Wave Detectors
• Prospects for gravitational-wave polarization test from compact binary mergers with future ground-based detectors
• Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
• Mapping the Universe Expansion: Enabling percent-level measurements of the Hubble Constant with a single binary neutron-star merger detection
• Probing hybrid stars with gravitational waves via interfacial modes
• Spherically symmetric static black holes in Einstein-aether theory
• Gravitational wave signatures of PBH-generated baryon-dark matter coincidence
• Primordial Black Holes as Dark Matter: Constraints From Compact Ultra-Faint Dwarfs
• Detecting the gravitational wave memory effect with TianQin
• Optical and mechanical properties of ion-beam-sputtered Nb${}_2$O${}_5$ and TiO${}_2$-Nb${}_2$O${}_5$ thin films for gravitational-wave interferometers
• First constraint on the dissipative tidal deformability of neutron stars
• Hybrid stars with sequential phase transitions: the emergence of the g${}_2$ mode
• Probing Early Universe Supercooled Phase Transitions with Gravitational Wave Data
• Three-dimensional GRMHD Simulations of Rapidly Rotating Stellar Core-Collapse
• Frequency-domain waveform approximants capturing Doppler shifts
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Neutron star-black hole mergers in next generation gravitational-wave observatories
• Resonant Shattering Flares in Black Hole-Neutron Star and Binary Neutron Star Mergers
• Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Gravitational wave source localization for eccentric binary coalesce with a ground-based detector network
• Alternative possibility of GW190521: Gravitational waves from high-mass black hole-disk systems
• Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors
• Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
• Super-slow phase transition catalyzed by BHs and the birth of baby BHs
• Pre-merger alert to detect the very-high-energy prompt emission from binary neutron-star mergers: Einstein Telescope and Cherenkov Telescope Array synergy
• Characterization of binary black holes by heterogeneous gravitational-wave networks
• Gravitational Wave Signatures of Highly Magnetized Neutron Stars
• Jet Launching from Merging Magnetized Binary Neutron Stars with Realistic Equations of State
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• The equation of state and radial oscillations of neutron stars
• Gravitational wave inference on a numerical-relativity simulation of a black hole merger beyond general relativity
• Probing Stochastic Gravitational Wave Background from $SU(5)\times U(1{)}_{\chi }$ Strings in Light of NANOGrav 15-Year Data
• Universal features of gravitational waves emitted by superkick binary black hole systems
• Gravitational Waves as a Probe of Globular Cluster Formation and Evolution
• Detectability of QCD phase transitions in binary neutron star mergers: Bayesian inference with the next generation gravitational wave detectors
• Mechanical Ringdown Studies of Large-Area Substrate-Transferred GaAs/AlGaAs Crystalline Coatings
• Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals
• Accurate and Efficient Waveform Model for Precessing Binary Black Holes
• Inference of the neutron star equation of state from cosmological distances
• The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
• Triaxially-deformed Freely-precessing Neutron Stars: Continuous electromagnetic and gravitational radiation
• Gravitational-wave echoes from numerical-relativity waveforms via space-time construction near merging compact objects
• Model-Independent Radiative Symmetry Breaking and Gravitational Waves
• Observing binary black hole ringdowns by advanced gravitational wave detectors
• Methods and prospects for gravitational wave searches targeting ultralight vector boson clouds around known black holes
• Ultra-delayed neutrino-driven explosion of rotating massive-star collapse
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Exploring compact binary populations with the Einstein Telescope
• Constraining the Cosmic Strings Gravitational Wave Spectra in No Scale Inflation with Viable Gravitino Dark matter and Non Thermal Leptogenesis
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• Induced Gravitational Waves probing Primordial Black Hole Dark Matter with Memory Burden
• Thermal noise and mechanical loss of SiO${}_2$/Ta${}_2$O${}_5$ optical coatings at cryogenic temperatures
• Identification of Lensed Gravitational Waves with Deep Learning
• Weyl double copy and massless free fields in curved spacetimes
• Pulsar revival in neutron star mergers: multi-messenger prospects for the discovery of pre-merger coherent radio emission
• Flexible mapping of ringdown amplitudes for nonprecessing binary black holes
• Super heavy dark matter origin of the PeV neutrino event: KM3-230213A
• Quantum correlation measurements in interferometric gravitational wave detectors
• A statistical inference approach to time-delay interferometry for gravitational-wave detection
• Detecting the stochastic gravitational wave background with the TianQin detector
• Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom
• Theory-agnostic framework for inspiral tests of general relativity with higher-harmonic gravitational waves
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Non-Markovian open quantum system approach to the early universe: I. Damping of gravitational waves by matter
• Viewing angle constraints on S190425z and S190426c and the joint gravitational-wave/gamma-ray detection fractions for binary neutron star mergers
• Multi-wavelength observations of cosmological phase transitions using LISA and Cosmic Explorer
• Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA
• A Direct Approach for the Fluctuation-Dissipation Theorem under Non-Equilibrium Steady-State Conditions
• Projected constraints on the dispersion of gravitational waves using advanced ground- and space-based interferometers
• The permanent ellipticity of the neutron star in PSR J1023+0038
• Searching for High Frequency Gravitational Waves with Phonons
• Neutron Star$-$Neutron Star and Neutron Star$-$Black Hole Mergers: Multiband Observations and Early Warnings
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Distinguishing general relativity from Chern-Simons gravity using gravitational wave polarizations
• Probing Miracle-less WIMP Dark Matter via Gravitational Waves Spectral Shapes
• Gravitational waves from melting cosmic strings
• Of Harbingers and Higher Modes: Improved gravitational-wave early-warning of compact binary mergers
• Parameter estimation methods for analyzing overlapping gravitational wave signals in the third-generation detector era
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Precision constraints on the neutron star equation of state with third-generation gravitational-wave observatories
• Limits on Runaway Growth of Intermediate Mass Black Holes from Advanced LIGO
• Tidal Love numbers and approximate universal relations for fermion soliton stars
• Synthetic FM triplet for AM-free precision laser stabilization and spectroscopy
• Particle swarm optimization of the sensitivity of a cryogenic gravitational wave detector
• Wave effect of gravitational waves intersected with a microlens field: a new algorithm and supplementary study
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Repulsive properties of hadrons in lattice QCD data and neutron stars
• Converting the signal-recycling cavity into an unstable optomechanical filter to enhance the detection bandwidth of gravitational-wave detectors
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Frequency space derivation of linear and non-linear memory gravitational wave signals from eccentric binary orbits
• Binary white dwarfs and decihertz gravitational wave observations: From the Hubble constant to supernova astrophysics
• Improvements in Gravitational-Wave Sky Localization with Expanded Networks of Interferometers
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• On arrival time difference between lensed gravitational waves and light
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity
• Unbiased likelihood-free inference of the Hubble constant from light standard sirens
• Dynamical tides during the inspiral of rapidly spinning neutron stars: Solutions beyond mode resonance
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• Tidal heating as a direct probe of strangeness inside neutron stars
• Quasinormal Modes for Dynamical Black Holes
• Constraining the Extra Polarization Modes of Gravitational Waves with Double White Dwarfs
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• Searching for spin-2 ULDM with gravitational waves interferometers
• Prospects for detecting transient quasi-monochromatic gravitational waves from glitching pulsars with current and future detectors
• Synergy between ground and space based gravitational wave detectors II: Localisation
• Calibration Uncertainty's Impact on Gravitational-Wave Observations
• Signatures of a High Temperature QCD Transition in the Early Universe
• Induced Gravitational Waves from Multi-Sound Speed Resonances during Cosmological Inflation
• Gravitational Waves from Phase Transition in Minimal SUSY $U(1{)}_{B-L}$ Model
• Spontaneous Scalarization as a New Core-Collapse Supernova Mechanism and its Multi-Messenger Signals
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Extended reduced-order surrogate models for scalar-tensor gravity in the strong field and applications to binary pulsars and gravitational waves
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies
• Accretion-modified stellar-mass black hole distribution and milli-Hz gravitational wave backgrounds from galaxy centre
• High-Precision Ringdown Surrogate Model for Non-Precessing Binary Black Holes
• Probing Left-Right Symmetry via Gravitational Waves from Domain Walls
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• Gravitational Wave Astronomy: Delivering on the Promises
• Gravitational waves from burdened primordial black holes dark matter
• Observing cosmological binary mergers with next generation neutrino and gravitational wave detectors
• PeV-Scale SUSY and Cosmic Strings from F-term Hybrid Inflation
• Multimessenger Emission from the Accretion Induced Collapse of White Dwarfs
• Application of the Hilbert-Huang transform for analyzing standing-accretion-shock-instability induced gravitational waves in a core-collapse supernova
• D-term inflation in braneworld models: Consistency with cosmic-string bounds and early-time Hubble tension resolving models
• Glitch subtraction from gravitational wave data using adaptive spline fitting
• Resolving phase transition properties of dense matter through tidal-excited g-mode from inspiralling neutron stars
• Stability of the protoneutron stars toward black hole formation
• Probing general relativistic spin-orbit coupling with gravitational waves from hierarchical triple systems
• Tidal deformability and gravitational-wave phase evolution of magnetised compact-star binaries
• Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
• Characterization of Laser Systems at 1550 nm Wavelength for Future Gravitational Wave Detectors
• An arm length stabilization system for KAGRA and future gravitational-wave detectors
• The lure of sirens: joint distance and velocity measurements with third generation detectors
• Gravitational Wave Opacity from Gauge Field Dark Energy
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Mergers of Maximally Charged Primordial Black Holes
• Dark Matter Signals on a Laser Interferometer
• Gravitational Waves from Peaks
• Neutron Star Structure in the Minimal Gravitational Standard-Model Extension and the Implication to Continuous Gravitational Waves
• The impact of dark matter on tidal signatures in neutron star mergers with Einstein Telescope
• Accuracy of source localization for eccentric inspiraling binary mergers using a ground-based detector network
• Heavy dark matter and Gravitational waves
• Multimessenger astronomy with a kHz-band gravitational-wave observatory
• Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• Performance-Portable Binary Neutron Star Mergers with AthenaK
• Imprint of PBH domination on gravitational waves generated by cosmic strings
• Strong gravity signatures in the polarization of gravitational waves
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Gravitational waves from cosmic strings associated with pseudo-Nambu-Goldstone dark matter
• An Empirical Study of Contamination in Deep, Rapid, and Wide-Field Optical Follow-Up of Gravitational Wave Events
• Possible binary neutron star merger history of the primary of GW230529
• Improved inspiral-merger-ringdown model for BBHs on elliptical orbits
• Gravitational wave asteroseismology limits from low density nuclear matter and perturbative QCD
• Learning orbital dynamics of binary black hole systems from gravitational wave measurements
• Tomography of flavoured leptogenesis with primordial blue gravitational waves
• On the detection of the electromagnetic counterparts from lensed gravitational wave events by binary neutron star mergers
• Measurement of the Cross-Correlation Angular Power Spectrum Between the Stochastic Gravitational Wave Background and Galaxy Over-Density
• Radio Afterglows from Compact Binary Coalescences: Prospects for Next-Generation Telescopes
• Improved early warning of compact binary mergers using higher modes of gravitational radiation: A population study
• Frequency-dependent squeezing for gravitational-wave detection through quantum teleportation
• Phase-transition sound of inflation at gravitational waves detectors
• Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
• Calibrating gravitational-wave detectors with GW170817
• Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models
• Numerical Inside View of Hypermassive Remnant Models for GW170817
• On Detecting Stellar Binary Black Holes via the LISA-Taiji Network
• Observing the dark sector
• Infinitely degenerate exact Ricci-flat solutions in f(R) gravity
• Rotational-tidal phasing of the binary neutron star waveform
• Probing the Fermi-LAT GeV excess with gravitational waves
• The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars
• Weak lensing of gravitational waves in wave optics: Beyond the Born approximation
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
• Constraining the delay time distribution of compact binary objects from the stochastic gravitational wave background searches
• Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
• Black Hole Formation and Explosion from Rapidly Rotating Very Massive Stars
• Optical and mechanical properties of ion-beam-sputtered MgF${}_2$ thin films for gravitational-wave interferometers
• Constraining the history of reheating with the NANOGrav 15-year data
• Unveiling the Nature of Gravitational-Wave Emission in Core-collapse Supernovae with Perturbative Analysis
• Microlensing bias on the detection of strong lensing gravitational wave
• Enhancing interferometer sensitivity without sacrificing bandwidth and stability: beyond single-mode and resolved-sideband approximation
• Detectability of gravitational higher order modes in the third-generation era
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Impact of unmodeled eccentricity on the tidal deformability measurement and implications for gravitational wave physics inference
• Detection of Gravitational Waves using Parametric Resonance in Bose-Einstein Condensates
• Bubble wall velocity and gravitational wave in the minimal left-right symmetric model
• Improvement of the parameter measurement accuracy by the third-generation gravitational wave detector Einstein Telescope
• Superconducting Levitated Detector of Gravitational Waves
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Simulation-based inference of black hole ringdowns in the time domain
• Postmerger multimessenger analysis of binary neutron stars: Effect of the magnetic field strength and topology
• Implications for Cosmic Domain Walls from LIGO-Virgo First Three Observing Runs
• Constraining hierarchical mergers of binary black holes detectable with LIGO-Virgo
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• Premerger phenomena in neutron-star binary coalescences
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• Non-radial oscillations and gravitational wave emission of hybrid neutron stars
• Visualizing convolutional neural network for classifying gravitational waves from core-collapse supernovae
• A Broadband Signal Recycling Scheme for Approaching the Quantum Limit from Optical Losses
• An optimised gravitational wave follow-up strategy with the Australian Square Kilometre Array Pathfinder
• Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
• Parametrized tests of general relativity using eccentric compact binaries
• Signature of hadron-quark crossover in binary-neutron-star mergers
• Fundamental Relations between Measurement, Radiation and Decoherence in Gravitational Wave Laser Interferometer Detectors
• Prospecting bipartite Dark Matter through Gravitational Waves
• Dark photon bursts from compact binary systems and constraints
• Supernova and prompt gravitational-wave precursors to LIGO gravitational-wave sources and short-GRBs
• 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
• Gravitational wave cosmology I: high frequency approximation
• Early warning of precessing compact binary merger with third-generation gravitational-wave detectors
• Leptogenesis, Dark Matter and Gravitational Waves from Discrete Symmetry Breaking
• Host galaxy identification for binary black hole mergers with long baseline gravitational wave detectors
• Exploring Fermionic Dark Matter Admixed Neutron Stars in the Light of Astrophysical Observations
• Detectability of stochastic gravitational wave background from weakly hyperbolic encounters
• Kerr-Enhanced Optical Spring
• Probing Spin-Induced Quadrupole Moments in Precessing Compact Binaries
• Wave effect of gravitational waves intersected with a microlens field II: an adaptive hierarchical tree algorithm and population study
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• Outliers in the LIGO Black Hole Mass Function from Coagulation in Dense Clusters
• An interference-based method for the detection of strongly lensed gravitational waves
• Distinguishing a stochastic gravitational-wave signal from correlated noise with joint parameter estimation: Fisher analysis for ground-based detectors
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Effects of mirror birefringence and its fluctuations to laser interferometric gravitational wave detectors
• Inferring Interference: Identifying a Perturbing Tertiary with Eccentric Gravitational Wave Burst Timing
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Searching for wormholes with gravitational wave scattering
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• Probing the impact of Delta-Baryons on Nuclear Matter and Non-Radial Oscillations in Neutron Stars
• Were recently reported MHz events planet mass primordial black hole mergers?
• The appearance of a merging binary black hole very close to a spinning supermassive black hole
• Tracing Astrophysical Black Hole Seeds and Primordial Black Holes with LISA-Taiji Network
• General relativistic surface degrees of freedom in perturbed hybrid stars
• Transition from inspiral to plunge for braneworld EMRI
• Signatures of Quantum Gravity in the Gravitational Self-Interaction of Photons
• Associating fast radio bursts with compact binary mergers via gravitational lensing
• Fundamental Physics and Cosmology with TianQin
• Effects of Galaxy Cluster Structure on Lensed Gravitational Waves
• Early warning of precessing neutron-star black-hole binary mergers with the near-future gravitational-wave detectors
• Scalar polarization window in gravitational-wave signals
• Observable tensor-to-scalar ratio and secondary gravitational wave background
• Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes
• Universal relations to measure neutron star properties from targeted r-mode searches
• Gravitational Waves from Metastable Cosmic Strings in Supersymmetric New Inflation Model
• PeV-scale leptogenesis, gravity waves and black holes from a SUSY-breaking phase transition
• Tracking Down the Route to the SM with Inflation and Gravitational Waves
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Testing general relativity via direct measurement of black hole kicks
• Quantum Black Hole Seismology II: Applications to Astrophysical Black Holes
• Probing dark matter with polarimetry techniques
• The missing link in gravitational-wave astronomy: A summary of discoveries waiting in the decihertz range
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• HERMES: Gamma Ray Burst and Gravitational Wave counterpart hunter
• Evaporating black holes: constraints on anomalous emission mechanisms
• Broadband Quantum Noise Reduction in Future Long Baseline Gravitational-wave Detectors via EPR Entanglement
• Precessing Binary Black Holes as Better Dark Sirens
• Forecasting the population properties of merging black holes
• The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation
• Constraining gravitational-wave backgrounds from conversions into photons in the Galactic magnetic field
• Gravitational Waves of GUT Phase Transition during Inflation
• On the Expected Backreaction During Preheating
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• A Summary of Multimessenger Science with Neutron Star Mergers
• On the Testability of the Quark-Hadron Transition Using Gravitational Waves From Merging Binary Neutron Stars
• Mass and radius of the most massive neutron star: The probe of the equation of state and perturbative QCD
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Assessing the Impact of Unequal Noises and Foreground Modeling on SGWB Reconstruction with LISA
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• Design of a CubeSat Payload to Test a Magnetic Measurement System for Space-borne Gravitational Wave Detectors
• Left-Right Symmetry Breaking and Gravitational Waves : A Tale of Two Phase Transitions
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Astrophysics with the Laser Interferometer Space Antenna
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Binary dynamics from Einstein-Maxwell theory at second post-Newtonian order using effective field theory
• Constraining parameters of coalescing stellar mass binary black hole systems with the Einstein Telescope alone
• Probing Dark Star Parameters Through $f$-Mode Gravitational Wave Signals
• Polymer quantization and advanced gravitational wave detector
• Constraining the ellipticity and frequency of binary neutron star remnant via its gravitational-wave and electromagnetic radiations
• Displacement-noise-free neutron interferometer for gravitational wave detection using a single Mach-Zehnder configuration
• Relic Cosmological Vector Fields and Inflationary Gravitational Waves
• Lower limit on the entropy of black holes as inferred from gravitational wave observations
• Torsional oscillations of magnetized neutron stars with mixed poloidal-toroidal fields
• Relevance of Precession for Tests of the Black Hole No Hair Theorems
• Inferring small neutron star spins with neutron star-black hole mergers
• Gravitational waves from binary black holes as probes of the structure formation history
• Cosmology and the Early Universe
• Effects of inner crusts on $g$-mode oscillations in neutron stars
• Probing nontensorial gravitational waves with a next-generation ground-based detector network
• Gravitational Wave From Axion-like Particle Inflation
• First-order QCD transition in a primordial magnetic field
• Neutron displacement noise-free interferometer for gravitational-wave detection
• Corrections to the gravitational wave phasing
• Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform
• Unraveling the CMB lack-of-correlation anomaly with the cosmological gravitational wave background
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Exposing Gravitational Waves below the Quantum Shot Noise
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• X- and Gamma-ray astrophysics in the era of Multi-messenger astronomy
• Probing the formation of the seeds of supermassive black holes with gravitational waves
• Probing Particle Physics with Gravitational Waves
• Gravitational Waves from Supernova Mass Loss and Natal Kicks in Close Binaries
• Gravitational waves from quasielliptic compact binaries in scalar-tensor theory to one-and-a-half post-Newtonian order
• Multi-messenger observations in the Einstein Telescope era: binary neutron star and black hole - neutron star mergers
• Non perturbative spherical gravitational waves
• Tidal dissipation in binary neutron star inspirals from hyperon bulk viscosity: Phase modeling and parameter estimation bias
• Probing intermediate scale Froggatt-Nielsen models at future gravitational wave observatories
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone
• Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
• Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
• Effects of multidimensional treatment of gravity in simulations on supernova gravitational waves
• $M/R$ estimates for two neutron stars in LMXBs with possible r-mode frequencies detected
• Scalar Gravitational Wave Signals from Core Collapse in Massive Scalar-Tensor Gravity with Triple-Scalar Interactions
• Effect of Dark matter and $\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars
• The directional isotropy of LIGO-Virgo binaries
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Gravitational waves from superradiant instabilities of rotating black holes
• The Dawn of Black Holes
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Identifying multichannel coherent couplings and causal relationships in gravitational wave detectors
• Constraining self-interactions of a massive scalar field using scalar gravitational waves from stellar core collapse
• How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
• Detectability of the gravitational-wave background produced by magnetar giant flares
• Beyond the Long Wavelength Approximation: Next-generation Gravitational-Wave Detectors and Frequency-dependent Antenna Patterns
• Primordial Black Holes and Second-order Gravitational Waves in Axion-like Hybrid Inflation
• Atmospheric Newtonian noise modeling for third-generation gravitational wave detectors
• Sensing and vetoing loud transient noises for the gravitational-wave detection
• Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Self-calibration of Networks of Gravitational Wave Detectors
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Testing hilltop supernatural inflation with gravitational waves
• Cold Atoms in Space: Community Workshop Summary and Proposed Road-Map
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Probing the Dark Solar System: Detecting Binary Asteroids with a Space-Based Interferometric Asteroid Explorer
• Quantum sensors with matter waves for GW observation
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• Inflation, Proton Decay and Gravitational Waves from Metastable Strings in $SU(4{)}_C\times SU(2{)}_L\times U(1{)}_R$ Model
• Obtaining Statistical Significance of Gravitational Wave Signals in Hierarchical Search
• Continuous gravitational waves in the lab: recovering audio signals with a table-top optical microphone
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Reconstructing the star formation rate for compact binary populations with the Einstein telescope
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• Probing Fundamental Physics with Gravitational Waves
• Tail wavelets in the merger of binary compact objects
• Characterization of ion-beam-sputtered AlF${}_3$ thin films for gravitational-wave interferometers
• Imprints of the redshift evolution of double neutron star merger rate on the signal to noise ratio distribution
• Reduced order modelling in searches for continuous gravitational waves - I. Barycentering time delays
• TOrsion-Bar Antenna: A Ground-Based Detector for Low-Frequency Gravity Gradient Measurement
• Perspectives for multi-messenger astronomy with the next generation of gravitational-wave detectors and high-energy satellites
• Self-consistent treatment of thermal effects in neutron-star post-mergers: observational implications for third-generation gravitational-wave detectors
• Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star
• Rotations of the polarization of a gravitational wave propagating in Universe
• Fully general-relativistic simulations of isolated and binary strange quark stars
• Gravitational wave and dark matter from Axion-Higgs string
• Overlapping signals in next-generation gravitational wave observatories: A recipe for selecting the best parameter estimation technique
• The Supersonic Project: SIGOs, a Proposed Progenitor to Globular Clusters, and their Connections to Gravitational Wave Anisotropies
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks
• General relativistic hydrodynamic simulations of binary strange star mergers
• Bayesian Analysis of Wave-Optics Gravitationally Lensed Massive Black Hole Binaries with Space-Based Gravitational Wave Detector
• Verifiable type-III seesaw and dark matter in a gauged $\mathbf{U}(1{)}_{\mathrm{B}-\mathrm{L}}$ symmetric model
• Hierarchical searches for subsolar-mass binaries and the third-generation gravitational wave detector era
• Continuous gravitational waves from thermal mountains on accreting neutron stars: effect of the nuclear pasta phase
• Can the phase of radiation pressure fluctuations be flipped in a single path for laser interferometric gravitational wave detectors?
• Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy
• Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts
• Could the stochastic gravitational wave background from newborn magnetars be detected by the advanced LIGO and Einstein Telescope?
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors
• Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates
• Gravitational-wave echoes from spinning exotic compact objects: numerical waveforms from the Teukolsky equation
• High speed, high power 2D beam steering for mitigation of optomechanical parametric instability in gravitational wave detectors
• Probing Leptophobic Dark Sectors via Gravitational Wave Signatures
• Lepton parity dark matter and naturally unstable domain walls
• Importance of relativistic pericenter precession in identifying the presence of a third body near eccentric binaries
• Calibrating systematic errors in the distance determination with the luminosity-distance space large scale structure of dark sirens and its potential applications
• Lensing by primordial black holes: constraints from gravitational wave observations
• First-post-Newtonian generation of gravitational waves in Einstein-Cartan theory
• The landscape of massive black-hole spectroscopy with LISA and Einstein Telescope
• Modeling the Beam of Gravitational Radiation from a Cosmic String Loop
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Convection signatures in early-time gravitational waves from core-collapse supernovae
• Extremely High-Order Convergence in Simulations of Relativistic Stars
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• Massive black hole binaries in LISA: constraining cosmological parameters at high redshifts
• Probing baryogenesis with gravitational waves
• Complementary signatures of $\alpha -$attractor inflation in CMB and cosmic string Gravitational Waves
• Neutron star evolution by combining discontinuous Galerkin and finite volume methods
• Imprints of an early matter-dominated era arising from dark matter dilution mechanism on cosmic string dynamics and gravitational wave signatures
• Rigorous analytic solution to the gravitational-wave overlapping event rates
• Collapsing domain walls with ${\mathbb{Z}}_2$-violating coupling to thermalized fermions and their impact on gravitational wave detections
• Relative calibration of the LIGO and Virgo detectors using astrophysical events from their third observing run
• Tidal deformations of compact objects and gravitational wave emission
• Low-Frequency Noise Mitigation and Bandgap Engineering using Seismic Metamaterials for Terrestrial Gravitational Wave Observatories
• Testing Nambu-Goto approximation of cosmic string by lattice field simulations
• Gravitational Wave Mountains: current-carrying domain walls
• Detectability of the Phase Transition Gravitational Waves in the DFSZ axion Model
• Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Primordial gravitational waves: Model effects on time evolution and spectrum
• Null-stream-based Bayesian Unmodeled Framework to Probe Generic Gravitational-wave Polarizations
• Tidal Love numbers and the dynamical instability of AdS bubbles
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Linking gravitational waves and X-ray phenomena with joint LISA and Athena observations
• Assessing the Distance for Probing the Nuclear Equation of State with Supernova Gravitational Waves
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• Optimising the observation of optical kilonovae with medium size telescopes
• Mutated hilltop inflation in light of Planck/ACT observations
• Gravitational-wave standard sirens and application in cosmology
• Gravitational lensing of gravitational waves: universal characteristics of strongly lensed memory waveforms
• Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands
• Gravitational waves from parabolic encounters: A study of linear and nonlinear memory
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Intermediate-Mass Black Holes in Extragalactic Globular Clusters
• Capability for detection of GW190521-like binary black holes with TianQin
• Stochastic Gravitational-Wave Background from Stellar Core-Collapse Events
• Effective-one-body formalism for leading-order radiative effects in the post-linear framework
• Very-High-Frequency Gravitational Waves from Multi-Monodromy Inflation
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
• Probing High Scale Dirac Leptogenesis via Gravitational Waves from Domain Walls
• Gravitational wave background from mergers of large primordial black holes
• Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
• Kination cosmology from scalar fields and gravitational-wave signatures
• Dynamical double black holes and their host cluster properties
• Detector induced anisotropies on the angular distribution of gravitational wave sources and opportunities of constraining horizon scale anisotropies
• Impact of Higher-order Tidal Corrections on the Measurement Accuracy of Neutron Star Tidal Deformability
• Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
• Initial acquisition requirements for optical cavities in the space gravitational wave antennae DECIGO and B-DECIGO
• Covariant transverse-traceless projection for secondary gravitational waves
• Multi-detector characterization of gravitational-wave burst tensor polarizations with the BayesWave algorithm
• Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
• Updated estimates of post-merger gravitational wave energy released in GW170817 and the maximum neutron star mass
• Linking the KM3-230213A Neutrino Event to Dark Matter Decay and Gravitational Wave signals