Binary Black Hole Mergers in the first Advanced LIGO Observing Run

Abstract

The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2016, saw the first detections of gravitational waves from binary black hole mergers. In this paper we present full results from a search for binary black hole merger signals with total masses up to $100M_{\odot }$ and detailed implications from our observations of these systems. Our search, based on general-relativistic models of gravitational wave signals from binary black hole systems, unambiguously identified two signals, GW150914 and GW151226, with a significance of greater than $5\sigma$ over the observing period. It also identified a third possible signal, LVT151012, with substantially lower significance, and with an 87% probability of being of astrophysical origin. We provide detailed estimates of the parameters of the observed systems. Both GW150914 and GW151226 provide an unprecedented opportunity to study the two-body motion of a compact-object binary in the large velocity, highly nonlinear regime. We do not observe any deviations from general relativity, and place improved empirical bounds on several high-order post-Newtonian coefficients. From our observations we infer stellar-mass binary black hole merger rates lying in the range $9-240{\mathrm{Gpc}}^{-3}{\mathrm{yr}}^{-1}$. These observations are beginning to inform astrophysical predictions of binary black hole formation rates, and indicate that future observing runs of the Advanced detector network will yield many more gravitational wave detections.

arXiv comment36 pages + 4 appendices, 14 figures; updated author list and references, final journal version, with appended Erratum for figures 7 and 8

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• Center-of-mass angular momentum and memory effect in asymptotically flat spacetimes
• Searching for the full symphony of black hole binary mergers
• Frequency-Dependent Responses in 3rd Generation Gravitational-Wave Detectors
• The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae
• Primordial Black Holes
• Resonant Tidal Excitation of Oscillation Modes in Merging Binary Neutron Stars: Inertial-Gravity Modes
• Gravitational wave signal recognition of O1 data by deep learning
• Neutron star mergers as a probe of modifications of general relativity with finite-range scalar forces
• Constraining the primordial black hole abundance with 21cm cosmology
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• Spin-Orbit Misalignment of Merging Black-Hole Binaries with Tertiary Companions
• Bounding the speed of gravity with gravitational wave observations
• Modeling the source of GW150914 with targeted numerical-relativity simulations
• Dynamics of black hole - neutron star binaries in young star clusters
• Tests of General Relativity with Gravitational-Wave Observations using a Flexible--Theory-Independent Method
• Fixing extensions to General Relativity in the non-linear regime
• Science with the TianQin observatory: Preliminary results on testing the no-hair theorem with ringdown signals
• Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• The second RIT binary black hole simulations catalog and its application to gravitational waves parameter estimation
• Electromagnetic signals following stellar-mass black hole mergers
• Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-Based Cross-Correlation Search in Advanced LIGO Data
• The optimal search for an astrophysical gravitational-wave background
• The effect of matter structure on the gravitational waveform
• What is a singular black hole beyond General Relativity?
• Parameterized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method
• Fast and Accurate Sensitivity Estimation for Continuous-Gravitational-Wave Searches
• Consistent relativistic mean field models constrained by GW170817
• Hidden universality in the merger rate distribution in the primordial black hole scenario
• Constraints on the primordial curvature power spectrum from primordial black holes
• Quasinormal-mode filters: a new approach to analyze the gravitational-wave ringdown of binary black-hole mergers
• Constraining the Inclination of Binary Mergers from Gravitational-wave Observations
• Cosmological inference using only gravitational wave observations of binary neutron stars
• Inferences about supernova physics from gravitational-wave measurements: GW151226 spin misalignment as an indicator of strong black-hole natal kicks
• Hierarchical test of general relativity with gravitational waves
• Gravitational Waves Probes of Parity Violation in Compact Binary Coalescence
• Probing Primordial-Black-Hole Dark Matter with Gravitational Waves
• Neutrino transport in black hole-neutron star binaries: neutrino emission and dynamical mass ejection
• Post-Kerr black hole spectroscopy
• Relativistic Dynamics and Mass Exchange in Binary Black Hole Mini-Disks
• Dynamical scalar hair formation around a Schwarzschild black hole
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Rush the inspiral: efficient Effective One Body time-domain gravitational waveforms
• Template-based Gravitational-Wave Echoes Search Using Bayesian Model Selection
• Numerical Relativity of Compact Binaries in the 21st Century
• Search for Gravitational Waves Associated with Gamma-Ray Bursts During the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B
• GW$\times$LSS: Chasing the Progenitors of Merging Binary Black Holes
• Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network
• Advanced quantum techniques for future gravitational-wave detectors
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• Effects of nonquadrupole modes in the detection and parameter estimation of black hole binaries with nonprecessing spins
• Accelerating gravitational wave parameter estimation with multi-band template interpolation
• Using gravitational-wave data to constrain dynamical tides in neutron star binaries
• The Third RIT binary black hole simulations catalog
• Looking at cosmic near-infrared background radiation anisotropies
• Binary Black Hole Mergers from LIGO/Virgo O1 and O2: Population Inference Combining Confident and Marginal Events
• Dynamical ejecta from precessing neutron star-black hole mergers with a hot, nuclear-theory based equation of state
• Eikonal quasinormal modes of black holes beyond General Relativity
• The electromagnetic chirp of a compact binary black hole: a phase template for the gravitational wave inspiral
• Detecting Gravitational Waves in Data with Non-Gaussian Noise
• Apples and Oranges: Comparing black holes in X-ray binaries and gravitational-wave sources
• Echoes from the braneworld black holes
• Does Matter Matter? Using the mass distribution to distinguish neutron stars and black holes
• Biases in parameter estimation from overlapping gravitational-wave signals in the third generation detector era
• The search for failed supernovae with the Large Binocular Telescope: a new candidate and the failed SN fraction with 11 yr of data
• Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes
• Accelerating parameter inference with graphics processing units
• Echoes from the Abyss: A highly spinning black hole remnant for the binary neutron star merger GW170817
• Validating gravitational-wave detections: The Advanced LIGO hardware injection system
• All-sky Search for Continuous Gravitational Waves from Isolated Neutron Stars in the Early O3 LIGO Data
• Distance and properties of NGC 4993 as the host galaxy of a gravitational wave source, GW170817
• Probing the nature of central objects in extreme-mass-ratio inspirals with gravitational waves
• A generalized precession parameter ${\chi }_{\mathrm{p}}$ to interpret gravitational-wave data
• Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
• Prospects for detecting gravitational waves at 5 Hz with ground-based detectors
• Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
• Importance of transient resonances in extreme-mass-ratio inspirals
• A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
• Black Hole Echology: The Observer's Manual
• An approach to computing spectral shifts for black holes beyond Kerr
• Implications of the low binary black hole aligned spins observed by LIGO
• Multi-mode black hole spectroscopy
• Solving post-Newtonian accurate Kepler Equation
• Two-harmonic approximation for gravitational waveforms from precessing binaries
• A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-Wave Detections
• Foliation dependence of black hole apparent horizons in spherical symmetry
• Exploring the high-redshift PBH-$\Lambda$CDM Universe: early black hole seeding, the first stars and cosmic radiation backgrounds
• Observational tests of the black hole area increase law
• Stellar binary black holes in the LISA band: a new class of standard sirens
• Single-single gravitational-wave captures in globular clusters: Eccentric deci-Hertz sources observable by DECIGO and Tian-Qin
• Gravitational wave energy emission and detection rates of Primordial Black Hole hyperbolic encounters
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• Revealing the formation of stellar-mass black hole binaries: The need for deci-Hertz gravitational wave observatories
• Constraining black hole mimickers with gravitational wave observations
• The merger history of primordial-black-hole binaries
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• Renormalized stress-energy tensor of an evaporating spinning black hole
• Dependence of Gravitational Wave Transient Rates on Cosmic Star Formation and Metallicity Evolution History
• Radiation reaction for spinning bodies in effective field theory II: Spin-spin effects
• Polarization test of gravitational waves from compact binary coalescences
• Constraints on compact dark matter from gravitational wave microlensing
• Parameter estimation for black hole echo signals and their statistical significance
• Illuminating the dark ages: Cosmic backgrounds from accretion onto primordial black hole dark matter
• Unbiased Hubble constant estimation from binary neutron star mergers
• Radiation reaction for spinning bodies in effective field theory I: Spin-orbit effects
• The NANOGrav 12.5-year data set: Search for Non-Einsteinian Polarization Modes in theGravitational-Wave Background
• Hairy binary black holes in Einstein-Maxwell-dilaton theory and their effective-one-body description
• Signatures of extra dimensions in gravitational waves from black hole quasi-normal modes
• Formation of primordial black holes in an axionlike curvaton model
• Tracking black hole kicks from gravitational wave observations
• Black Hole Pulsar
• GW170817/GRB 170817A/AT2017gfo association: some implications for physics and astrophysics
• Modeling ringdown II: non-precessing binary black holes
• PBH remnants as dark matter produced in thermal, matter and runaway-quintessence post-inflationary scenarios
• Astronomical tests for quantum black hole structure
• Effectual gravitational-wave template banks for coalescing compact binaries using a hybrid placement algorithm
• A self-consistent method to estimate the rate of compact binary coalescences with a Poisson mixture model
• Gravitational-wave cosmography with LISA and the Hubble tension
• Primordial Black Holes from Confinement
• Accreting black hole binaries in globular clusters
• The stochastic gravitational-wave background in the absence of horizons
• Binary Stars in the New Millennium
• Tidal Love Numbers of Black Holes and Neutron Stars in the Presence of Higher Dimensions: Implications of GW170817
• Data quality up to the third observing run of Advanced LIGO: Gravity Spy glitch classifications
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• Bimodal Long-Lasting Components in Short Gamma-Ray Bursts: Promising Electromagnetic Counterparts to Neutron Star Binary Mergers
• Probing Gravitational Parity Violation with Gravitational Waves from Stellar-mass Black Hole Binaries
• Nonlinear/non-iterative treatment of EFT-motivated gravity
• Constraining black-hole spins with gravitational wave observations
• Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations
• Primordial-black-hole mergers in dark-matter spikes
• Unraveling the origin of black holes from effective spin measurements with LIGO-Virgo
• Possible Causes of False General Relativity Violations in Gravitational Wave Observations
• Constraining alternative theories of gravity using pulsar timing arrays
• In-depth analysis of the clustering of dark matter particles around primordial black holes I: density profiles
• PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events
• Spontaneous scalarization of Gauss-Bonnet black holes: Analytic treatment in the linearized regime
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Testing the multipole structure of compact binaries using gravitational wave observations
• Confronting Models of Massive Star Evolution and Explosions with Remnant Mass Measurements
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• A Unique Multi-Messenger Signal of QCD Axion Dark Matter
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Angular momentum transport in massive stars and natal neutron star rotation rates
• Hamiltonian Formulation of the Conservative Self-Force Dynamics in the Kerr Geometry
• A "no-hair" test for binary black holes
• Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities
• Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
• Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems
• Coincident f(Q) gravity: black holes, regular black holes and black bounces
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• Ergoregion instability and echoes for braneworld black holes: Scalar, electromagnetic and gravitational perturbations
• On combining information from multiple gravitational wave sources
• Denoising of gravitational wave signals via dictionary learning algorithms
• A Bayesian Framework to Constrain the Photon Mass with a Catalog of Fast Radio Bursts
• Existence and Instability of Novel Hairy Black Holes in Shift-symmetric Horndeski Theories
• Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone
• Measuring the propagation speed of gravitational waves with LISA
• Numerical simulation of sky localization for LISA-TAIJI joint observation
• Ultrahigh-energy neutrino follow-up of Gravitational Wave events GW150914 and GW151226 with the Pierre Auger Observatory
• Deep learning and Bayesian inference of gravitational-wave populations: Hierarchical black-hole mergers
• Expanding the LISA Horizon from the Ground
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• The hangup effect in unequal mass binary black hole mergers and further studies of their gravitational radiation and remnant properties
• Echoes of novel black-bounce spacetimes
• Testing General Relativity with Gravitational Waves: An Overview
• Detectability of thermal neutrinos from binary-neutron-star mergers and implication to neutrino physics
• Strong constraints on clustered primordial black holes as dark matter
• Gravitational wave echoes from black holes in massive gravity
• Absorption of electromagnetic and gravitational waves by Kerr black holes: Shadows, superradiance and the spin-helicity effect
• Quasi-normal mode frequencies and gravitational perturbations of black holes with any subextremal spin in modified gravity through METRICS: the scalar-Gauss-Bonnet gravity case
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
• Predicting Stellar-Mass Black Hole Populations in Globular Clusters
• Primordial black holes and gravitational waves in nonstandard cosmologies
• The host galaxies of double compact objects merging in the local Universe
• Measuring precession in asymmetric compact binaries
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• Challenges testing the no-hair theorem with gravitational waves
• Mapping Incoherent Gravitational Wave Backgrounds
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Follow-up signals from superradiant instabilities of black hole merger remnants
• Maximum redshift of gravitational wave merger events
• Testing Gravity with Gravitational Waves from Binary Black Hole Mergers: Contributions from Amplitude Corrections
• A New Spin on an Old Black Hole: NuSTAR Spectroscopy of EXO 1846-031
• Scalar Hairy Black Holes in Four Dimensions are Unstable
• On the four-loop static contribution to the gravitational interaction potential of two point masses
• Brans-Dicke theory in Bondi-Sachs form: Asymptotically flat solutions, asymptotic symmetries and gravitational-wave memory effects
• Condensate of Massive Graviton and Dark Matter
• Pure polarization test of GW170814 and GW170817 using waveforms consistent with modified theories of gravity
• The mass quadrupole moment of compact binary systems at the fourth post-Newtonian order
• VAMANA: Modeling Binary Black Hole Population with Minimal Assumptions
• Prospects of detecting the nonlinear gravitational wave memory
• Gravitational-wave memory effects in Brans-Dicke theory: Waveforms and effects in the post-Newtonian approximation
• On the interpretation of the Fermi GBM transient observed in coincidence with LIGO Gravitational Wave Event GW150914
• Accretion-induced spin-wandering effects on the neutron star in Scorpius X-1: Implications for continuous gravitational wave searches
• Self-consistent semi-analytic models of the first stars
• Quasinormal Modes of a Black Hole with Quadrupole Moment
• Dynamics of binary black holes in low-mass young star clusters
• Detection of Gravitational Waves Using Bayesian Neural Networks
• A Fermi Gamma-ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-Wave Candidates in Advanced LIGO's First Observing Run
• Implications of the NANOGrav result on primordial gravitational waves in nonstandard cosmologies
• Parameter estimation of stellar-mass black hole binaries with LISA
• Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes
• Sensitivity of gravitational wave searches to the full signal of intermediate mass black hole binaries during the LIGO O1 Science Run
• Astrometric Effects of Gravitational Wave Backgrounds with non-Einsteinian Polarizations
• Constraining the parameters of GW150914 & GW170104 with numerical relativity surrogates
• Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins
• Black hole shadows in fourth-order conformal Weyl gravity
• Template Bank for Compact Binary Coalescence Searches in Gravitational Wave Data: A General Geometric Placement Algorithm
• Spin-induced deformations and tests of binary black hole nature using third-generation detectors
• Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube
• Simulations predict intermediate-mass black hole formation in globular clusters
• The Star Formation History of the Milky Way's Nuclear Star Cluster
• The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• The modification of photon trapping orbits as a diagnostic of non-Kerr spacetimes
• Prospects of Finding Detached Black Hole-Star Binaries with TESS
• Quasinormal modes, echoes and the causal structure of the Green's function
• Black Hole Superradiance in the Presence of Lorentz Symmetry Violation
• Parametrized tests of post-Newtonian theory using principal component analysis
• Tests of general relativity with stellar-mass black hole binaries observed by LISA
• Geometric Approach to Circular Photon Orbits and Black Hole Shadows
• Reconstruction of Primordial Power Spectrum of curvature perturbation from the merger rate of Primordial Black Hole Binaries
• Impact of Numerical Relativity information on effective-one-body waveform models
• Improved limits on a stochastic gravitational-wave background and its anisotropies from Advanced LIGO O1 and O2 runs
• New binary black hole mergers in the LIGO-Virgo O3b data
• Recognizing black holes in gravitational-wave observations: Challenges in telling apart impostors in mass-gap binaries
• Accurate inspiral-merger-ringdown gravitational waveforms for non-spinning black-hole binaries including the effect of subdominant modes
• Constraints on $f(R)$ theories of gravity from GW170817
• New Exact Spherically Symmetric Solutions in $f(R,\varphi ,X)$ gravity by Noether's symmetry approach
• Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
• Very fast stochastic gravitational wave background map making using folded data
• Spin-orbit precession for eccentric black hole binaries at first order in the mass ratio
• Second post-Newtonian order radiative dynamics of inspiralling compact binaries in the Effective Field Theory approach
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• A tale of two transients: GW170104 and GRB170105A
• When black holes collide: Probing the interior composition by the spectrum of ringdown modes and emitted gravitational waves
• An effective action model of dynamically scalarizing binary neutron stars
• Testing Gravitational Memory Generation with Compact Binary Mergers
• Lifetime of short-period binaries measured from their Galactic kinematics
• Detecting Kozai-Lidov imprints on the gravitational waves of intermediate-mass black holes in galactic nuclei
• On modeling for Kerr black holes: Basis learning, QNM frequencies, and spherical-spheroidal mixing coefficients
• Viewing angle of binary neutron star mergers
• Scattering of gravitational waves off spinning compact objects with an effective worldline theory
• Black hole spins in coalescing binary black holes
• Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
• Gravitational-wave Merger Forecasting: Scenarios for the early detection and localization of compact-binary mergers with ground based observatories
• Localization of binary mergers with gravitational-wave detectors of second and third generation
• Extended Cuscuton as Dark Energy
• News from horizons in binary black hole mergers
• Spectral method for metric perturbations of black holes: Kerr background case in general relativity
• Characterisation of lensing selection effects for LISA massive black hole binary mergers
• A synthetic model of the gravitational wave background from evolving binary compact objects
• Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
• The observed mass distribution of Galactic black hole LMXBs is biased against massive black holes
• Populating the Black Hole Mass Gaps In Stellar Clusters: General Relations and Upper Limits
• Probing beyond-Kerr spacetimes with inspiral-ringdown corrections to gravitational waves
• Archival searches for stellar-mass binary black holes in LISA
• Spectral Method for the Gravitational Perturbations of Black Holes: Schwarzschild Background Case
• Angular emission patterns of remnant black holes
• Probing Einstein-dilaton Gauss-Bonnet Gravity with the inspiral and ringdown of gravitational waves
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• Finite tidal effects in GW170817: Observational evidence or model assumptions?
• Impact of a Spinning Supermassive Black Hole on the Orbit and Gravitational Waves of a Nearby Compact Binary
• Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars
• Correlations in gravitational-wave reconstructions from eccentric binaries: A case study with GW151226 and GW170608
• Systematic errors in estimation of gravitational-wave candidate significance
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• The Unprecedented Properties of the First Electromagnetic Counterpart to a Gravitational Wave Source
• Gravitational-wave selection effects using neural-network classifiers
• Multiband Gravitational Wave Parameter Estimation: A Study of Future Detectors
• Puncture Initial Data for Black-Hole Binaries with High Spins and High Boosts
• The Effect of Distant Encounters on Black Hole Binaries in Globular Clusters: Systematic Increase of In-cluster Mergers in the LISA band
• Black hole superradiant instability for massive spin-2 fields
• All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run
• Metamorphoses of a photon sphere
• Methods for the detection of gravitational waves from sub-solar mass ultracompact binaries
• Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory
• Dark matter component in hadronic models with short-range correlations
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• Algorithm for TDI numerical simulation and sensitivity investigation
• A Single Progenitor Model for GW150914 and GW170104
• Inferring the core-collapse supernova explosion mechanism with three-dimensional gravitational-wave simulations
• Optical follow-up of gravitational wave events during the second advanced LIGO/VIRGO observing run with the DLT40 Survey
• Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA
• Tidal heating of Quantum Black Holes and their imprints on gravitational waves
• Curvatures, Photon Spheres and Black Hole Shadows
• Testing general relativity using binary extreme-mass-ratio inspirals
• On the Potential Observation of False Deviations from General Relativity in Gravitational Wave Observations from Binary Black Holes
• Localization of transient gravitational wave sources: beyond triangulation
• Measuring stochastic gravitational-wave energy beyond general relativity
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Systematic errors in estimation of gravitational-wave candidate significance
• Dynamics of binary black holes in young star clusters: the impact of cluster mass and long-term evolution
• The Lamb shift and the gravitational binding energy for binary black holes
• Optimal Generators for Quantum Sensing
• Dark particle mass effects on neutron star properties from a short-range correlated hadronic model
• Rapid and Robust Parameter Inference for Binary Mergers
• Investigating the relation between gravitational wave tests of general relativity
• Lensing of Gravitational Waves as a Novel Probe of Graviton Mass
• Gravitational-wave merging events from the dynamics of stellar mass binary black holes around the massive black hole in a galactic nucleus
• Prospects for gravitational-wave polarization test from compact binary mergers with future ground-based detectors
• Assessing the Energetics of Spinning Binary Black Hole Systems
• On the propagation of gravitational waves in strong magnetic fields
• Constraining accretion efficiency in massive binary stars with LIGO-Virgo black holes
• Bardeen solution with a cloud of strings
• Towards a framework for testing general relativity with extreme-mass-ratio-inspiral observations
• Inference-optimized AI and high performance computing for gravitational wave detection at scale
• Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• Multi-band gravitational wave astronomy: science with joint space- and ground-based observations of black hole binaries
• New inhomogeneous universes in scalar-tensor and f(R) gravity
• Comparing Remnant Properties from Horizon Data and Asymptotic Data in Numerical Relativity
• Electromagnetic precursor flares from the late inspiral of neutron star binaries
• Sub-threshold binary neutron star search in Advanced LIGO's first observing run
• Measuring the Speed of Gravitational Waves from the First and Second Observing Run of Advanced LIGO and Advanced Virgo
• Where and when: optimal scheduling of the electromagnetic follow-up of gravitational-wave events based on counterpart lightcurve models
• Targeted numerical simulations of binary black holes for GW170104
• Bayesian reconstruction of gravitational wave bursts using chirplets
• Formation of trapped vacuum bubbles during inflation, and consequences for PBH scenarios
• Self-intersecting marginally outer trapped surfaces
• Signatures of primordial black holes in gravitational wave clustering
• Nonlocality amplifies echoes
• Theory-agnostic framework for dynamical scalarization of compact binaries
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Frequency-domain waveform approximants capturing Doppler shifts
• The minimum and maximum gravitational-wave background from supermassive binary black holes
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
• Tidal heating of black holes and exotic compact objects on the brane
• Exploration of co-sputtered Ta${}_2$O${}_5$-ZrO${}_2$ thin films for gravitational-wave detectors
• Enhancing confidence in the detection of gravitational waves from compact binaries using signal coherence
• Constraints on the contributions to the observed binary black hole population from individual evolutionary pathways in isolated binary evolution
• Microlensing constraints on clustered primordial black holes
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue
• Gravitational-wave population inference at past time infinity
• Spontaneous scalarization with an extremely massive field and heavy neutron stars
• Systematic challenges for future gravitational wave measurements of precessing binary black holes
• A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
• Three observational differences for binary black holes detections with second and third generation gravitational-wave detectors
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Looking for extra dimensions in the observed quasi-periodic oscillations of black holes
• Exploring non-singular black holes in gravitational perturbations
• Scalar-tensor mixed polarization search of gravitational waves
• Characterization of binary black holes by heterogeneous gravitational-wave networks
• Eccentric Mergers in AGN Discs: Influence of the Supermassive Black-Hole on Three-body Interactions
• The nonspinning binary black hole merger scenario revisited
• Constraining alternative theories of gravity using GW$150914$ and GW$151226$
• Particle motion around a static axially symmetric wormhole
• Ultimate fate of apparent horizons during a binary black hole merger II: Horizons weaving back and forth in time
• NIR Counterparts to ULXs (III): Completing the photometric survey and selected spectroscopic results
• Sharp turns in axion monodromy: primordial black holes and gravitational waves
• Gravitational Wave Background Sky Maps from Advanced LIGO O1 Data
• Rapidly Rising Optical Transients from the Birth of Binary Neutron Stars
• Eccentricity distributions of eccentric binary black holes in galactic nuclei
• Rotating black hole mimicker surrounded by the string cloud
• Nested sampling cross-checks using order statistics
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Constraining Mixed Dark-Matter Scenarios of WIMPs and Primordial Black Holes from CMB and 21-cm observations
• Eccentric Binary Black Holes with Spin via the Direct Integration of the Post-Newtonian Equations of Motion
• Testing General Relativity with Black Hole-Pulsar Binaries
• Discovering the interior of black holes
• Correlated magnetic noise from anisotropic lightning sources and the detection of stochastic gravitational waves
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• Signatures of Einstein-Maxwell dilaton-axion gravity from the observed jet power and the radiative efficiency
• Implications of Einstein-Maxwell dilaton-axion gravity from the black hole continuum spectrum
• Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators
• Spherical symmetry as a test case for unconstrained hyperboloidal evolution II: gauge conditions
• The Gravitational Wave Stress-Energy (pseudo)-Tensor in Modified Gravity
• Quantum hair of black holes out of equilibrium
• New Gravitational Wave Discoveries Enabled by Machine Learning
• Imprint of black hole area quantization and Hawking radiation on inspiraling binary
• Revisiting time delay interferometry for unequal-arm LISA and TAIJI
• Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA
• Implementing Tidal and Gravitational Wave Energy Losses in Few-body Codes: A Fast and Easy Drag Force Model
• Are stellar--mass binary black hole mergers isotropically distributed?
• Projected constraints on the dispersion of gravitational waves using advanced ground- and space-based interferometers
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• Have hierarchical three-body mergers been detected by LIGO/Virgo?
• Evolution of black hole shadows from superradiance
• Tracking the origin of black holes with the stochastic gravitational wave background popcorn signal
• Probing Compactified Extra Dimensions with Gravitational Waves
• How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
• Limits on electromagnetic counterparts of gravitational wave-detected binary black hole mergers
• Secular evolution of compact binaries revolving around a spinning massive black hole
• Testing Vector Gravity with Gravitational Wave Interferometers
• Vector theory of gravity: Universe without black holes and solution of dark energy problem
• Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems
• Gravitational-Wave Background from Binary Mergers and Metallicity Evolution of Galaxies
• The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave Observatories
• Testing No-Hair Theorem by Quasi-Periodic Oscillations: the quadrupole of GRO J1655$-$40
• Self-force correction to geodetic spin precession in Kerr spacetime
• Probing the Black Hole Merger History in Clusters using Stellar Tidal Disruptions
• Analyzing clustering of astrophysical gravitational-wave sources: Luminosity-distance space distortions
• Light echos and coherent autocorrelations in a black hole spacetime
• On the Gravitational Wave Background from Black Hole Binaries after the First LIGO Detections
• The Exact Amplitudes of Six Polarization Modes for Gravitational Waves
• Gravitational wave constraints on planetary-mass primordial black holes using LIGO O3a data
• Astrophysical Prior Information and Gravitational-wave Parameter Estimation
• Ringing and echoes from black bounces surrounded by the string cloud
• Unmodelled Clustering Methods for Gravitational Wave Populations of Compact Binary Mergers
• Rainbow scattering in the gravitational field of a compact object
• Minimum energy and the end of the inspiral in the post-Newtonian approximation
• Evolution of diffuse scalar clouds around binary black holes
• A Search for Optical Emission from Binary-Black-Hole Merger GW170814 with the Dark Energy Camera
• Limits on Runaway Growth of Intermediate Mass Black Holes from Advanced LIGO
• Long gamma-ray burst rate at very high redshift
• About gravitational-wave generation by a three-body system
• Gödel-type solutions within the f(R,Q) gravity
• Probing intrinsic properties of short gamma-ray bursts with gravitational waves
• Constraining Screened Modified Gravity by Space-borne Gravitational-wave Detectors
• Stability of Hairy Black Holes in Shift-Symmetric Scalar-Tensor Theories via the Effective Field Theory Approach
• Multipole moments of compact objects with NUT charge: Theoretical and observational implications
• Electromagnetic Counterparts of Compact Binary Mergers
• Horizon Surface Gravity in Corotating Black Hole Binaries
• Decoherence of Gravitational Wave Oscillations in Bigravity
• Localization of Binary Black-Hole Mergers with Known Inclination
• Detection and characterization of spin-orbit resonances in the advanced gravitational wave detectors era
• Constraining the Extra Polarization Modes of Gravitational Waves with Double White Dwarfs
• The stepping-stone sampling algorithm for calculating the evidence of gravitational wave models
• Primordial black holes as dark matter and generators of cosmic structure
• Facilitating follow-up of LIGO-Virgo events using rapid sky localization
• Solar System tests and chameleon effect in f (R) gravity
• Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity
• Quasinormal Modes for Dynamical Black Holes
• Template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and the first observation run of Advanced Virgo
• Investigating the effect of in-plane spin directions for Precessing BBH systems
• Search for GeV Gamma-ray Counterparts of Gravitational Wave Events by CALET
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• The impact of selection biases on tests of general relativity with gravitational-wave inspirals
• Comment on "An excess of massive stars in the local 30 Doradus starburst"
• Detecting Gravitational Self Lensing from Stellar-Mass Binaries Composed of Black Holes or Neutron Stars
• A classifier for gravitational-wave inspiral signals in non-ideal single-detector data
• Numerical relativity higher order gravitational waveforms of eccentric, spinning, non-precessing binary black hole mergers
• Gravitational waves from neutron star excitations in binary inspirals
• Establishing the significance of continuous gravitational-wave detections from known pulsars
• Probing horizon scale quantum effects with Love
• Testing the Kerr nature of intermediate-mass and supermassive black hole binaries using spin-induced multipole moment measurements
• The MAVERIC Survey: Radio catalogs and source counts from deep Very Large Array imaging of 25 Galactic globular clusters
• Electromagnetic counterparts of high-frequency gravitational waves having additional polarization states: distinguishing and probing tensor-mode, vector-mode and scalar-mode gravitons
• Enhanced cosmological perturbations and the merger rate of PBH binaries
• Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment
• Extraction of black hole coalescence waveforms from noisy data
• Searching for primordial black holes with stochastic gravitational-wave background in the space-based detector frequency band
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• New search pipeline for gravitational waves with higher-order modes using mode-by-mode filtering
• Optimized Search for a Binary Black Hole Merger Population in LIGO-Virgo O3 Data
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Massive Graviton Geons
• Investigating the noise residuals around the gravitational wave event GW150914
• An axion-like scalar field environment effect on binary black hole merger
• Concurrent estimation of noise and compact-binary signal parameters in gravitational-wave data
• Primordial Black Hole Formation in Non-Standard Post-Inflationary Epochs
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Degeneracy of gravitational waveforms in the context of GW150914
• Matter Effects on LIGO/Virgo Searches for Gravitational Waves from Merging Neutron Stars
• Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
• Rotating Love: The dynamical tides of spinning Newtonian stars
• Enhancing the sensitivity of transient gravitational wave searches with Gaussian Mixture Models
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• On the primordial black hole formation in hybrid inflation
• Hierarchical Bayesian method for detecting continuous gravitational waves from an ensemble of pulsars
• Particle motion under the conservative piece of the self-force is Hamiltonian
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
• A blinding solution for inference from astronomical data
• Neutron star-black hole coalescence rate inferred from macronova/kilonova observations
• Positivity Bounds on parity-violating scalar-tensor EFTs
• Slowly Decaying Ringdown of a Rapidly Spinning Black Hole: Probing the No-Hair Theorem by Small Mass-Ratio Mergers with LISA
• Application of the third RIT binary black hole simulations catalog to parameter estimation of gravitational waves signals from the LIGO-Virgo O1/O2 observational runs
• Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars
• Assessing gravitational-wave binary black hole candidates with Bayesian odds
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• Conformal Killing horizons and their thermodynamics
• Estimating gravitational radiation from super-emitting compact binary systems
• Excitation of high frequency voices from intermediate-mass-ratio inspirals with large eccentricity
• Gravitational wave from warm inflation
• Measuring the primordial gravitational wave background in the presence of other stochastic signals
• Ranking Candidate Signals with Machine Learning in Low-Latency Search for Gravitational-Waves from Compact Binary Mergers
• Hunting electromagnetic counterparts of gravitational-wave events using the Zwicky Transient Facility
• Quasinormal modes and echo effect of cylindrical anti-de Sitter black hole spacetime with a thin shell
• Tidal Deformability of Strange Quark Planets and Strange Dwarfs
• Constraining the ellipticity of new-born magnetar with the observational data of Long gamma-ray bursts
• How would GW150914 look with future GW detector networks?
• Repeated mergers of black hole binaries: implications for GW190521
• Probing resonant excitations in exotic compact objects via gravitational waves
• Heavy-tailed likelihoods for robustness against data outliers: Applications to the analysis of gravitational wave data
• Characterization of low-significance gravitational-wave compact binary sources
• Enhancing the significance of gravitational wave bursts through signal classification
• Autoencoder-driven Spiral Representation Learning for Gravitational Wave Surrogate Modelling
• Observing the dark sector
• Bayesian inference for binary neutron star inspirals using a Hamiltonian Monte Carlo Algorithm
• Observational implications of lowering the LIGO-Virgo alert threshold
• Recipes for computing radiation from a Kerr black hole using a generalized Sasaki-Nakamura formalism: Homogeneous solutions
• Constraining the history of reheating with the NANOGrav 15-year data
• The ringing of quantum corrected Schwarzschild black hole with GUP
• Gravitational waves from merging intermediate-mass black holes : II Event rates at ground-based detectors
• Deciphering signatures of Bardeen black holes from the observed quasi-periodic oscillations
• Transition of EMRIs through resonance: corrections to higher order in the on-resonance flux modification
• INTEGRAL observations of GW170104
• A stochastic template bank for gravitational wave searches for precessing neutron-star--black-hole coalescence events
• An independent search of gravitational waves in the first observation run of advanced LIGO using cross-correlation
• Searching for compact objects in binaries with Gaia DR3
• Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• Gravitational Waves as a Probe of the Extra Dimension
• Constraining the impact of standard model phase transitions on primordial black holes
• An analysis and visualization of the output mode-matching requirements for squeezing in Advanced LIGO and future gravitational wave detectors
• New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
• Conformal gravity: light deflection revisited and the galactic rotation curve failure
• Astrophysical signal consistency test adapted for gravitational-wave transient searches
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• Simulations of Ellipsoidal Primordial Black Hole Formation
• Speeding Up Squeezing with a Periodically Driven Dicke Model
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Near-horizon chaos beyond Einstein gravity
• Bayesian Reconstruction of Gravitational-wave Signals from Binary Black Holes with Nonzero Eccentricities
• Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background
• Search for Coincident Gravitational-wave and Fast Radio Burst Events from 4-OGC and the First CHIME/FRB Catalog
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• GRB 111005A at Z = 0.0133 and the Prospect of Establishing Long-short GRB/GW Association
• Echoes of axial gravitational perturbations in stars of uniform density
• Strong-gravity precession resonances for binary systems orbiting a Schwarzschild black hole
• Neutrino emission upper limits with maximum likelihood estimators for joint astrophysical neutrino searches with large sky localizations
• Beyond general relativity: designing a template-based search for exotic gravitational wave signals
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• The growth of stellar mass black hole binaries trapped in an accretion disk of active galactic nuclei
• Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains
• Corral Framework: Trustworthy and Fully Functional Data Intensive Parallel Astronomical Pipelines
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Ringdown Spectroscopy of Rotating Black Holes Pierced by Cosmic Strings
• Primordial Black Holes without fine-tuning from a light stochastic spectator field
• Worldtube excision method for intermediate-mass-ratio inspirals: scalar-field model in 3+1 dimensions
• Motion of a spinning particle under the conservative piece of the self-force is Hamiltonian to first order in mass and spin
• Model-independent discovery prospects for primordial black holes at LIGO
• Gravitational-Wave Geodesy: A New Tool for Validating Detection of the Stochastic Gravitational-Wave Background
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers
• Black hole spectroscopy for KAGRA future prospect in O5
• Estimation of the gravitational wave polarizations from a non template search
• Sensors and Actuators for the Advanced LIGO+ Upgrade
• Waveforms from Amplitudes
• Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
• Transition from inspiral to plunge for braneworld EMRI
• How to confirm the existence of population III stars by observations of gravitational waves
• Detectability of Gravitational Wave from a population of Inspiralling Black Holes in Milky Way Mass Galaxies
• Black hole mass function and its evolution -- the first prediction for the Einstein Telescope
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Outflow-Driven Transients from the Birth of Binary Black Holes I: Tidally-Locked Secondary Supernovae
• Radio bounds on the mixed dark matter scenarios of primordial black holes and WIMPs
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Phenomenological Inclusion of Alternative Dispersion Relations to the Teukolsky Equation and its Application to Bounding the Graviton Mass with Gravitational-wave Measurements
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Outflow-Driven Transients from the Birth of Binary Black Holes II: Primary-Induced Accretion Transients
• Entangled Matter-waves for Quantum Enhanced Sensing
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• Scalar-Connection Gravity and Spontaneous Scalarization
• Consistent derivation of the Hawking effect for both non-extremal and extremal Kerr black holes
• Precessing Binary Black Holes as Better Dark Sirens
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Statistical properties of fast radio bursts elucidate their origins: magnetars are favoured over gamma-ray bursts
• Einstein-Klein-Gordon system via Cauchy-characteristic evolution: Computation of memory and ringdown tail
• Eccentricity matters: Impact of eccentricity on inferred binary black hole populations
• Lower limit on the entropy of black holes as inferred from gravitational wave observations
• Constraining parameters of coalescing stellar mass binary black hole systems with the Einstein Telescope alone
• Binary dynamics from Einstein-Maxwell theory at second post-Newtonian order using effective field theory
• Constraints on higher curvature gravity from time delay between GW170817 and GRB 170817A
• Identifying extra high frequency gravitational waves generated from oscillons with cuspy potentials using deep neural networks
• Stochastic inflation and non-perturbative power spectrum beyond slow roll
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• A Joint Ranking Statistic for Multi-messenger Astronomical Searches with Gravitational Waves
• New approach to template banks of gravitational waves with higher harmonics: Reducing matched-filtering cost by over an order of magnitude
• Gravitational multipole moments for asymptotically de Sitter spacetimes
• Probing the large-scale structure of the universe through gravitational-wave observations
• Rotating black holes in valid vector-tensor theories after GW170817
• Dipole Anisotropy in Gravitational Wave Source Distribution
• Inferring black-hole orbital dynamics from numerical-relativity gravitational waveforms
• Influence of tidal dissipation on outcomes of binary-single encounters between stars and black holes in stellar clusters
• Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer
• Can Primordial Black Holes form in the Standard Model ?
• Gödel-type Solutions in Cubic Galileon Gravity
• Geographic and seasonal influences on optical followup of gravitational wave events
• Driving unmodelled gravitational-wave transient searches using astrophysical information
• Constraining primordial black hole masses through $f(R)$ gravity scalarons in Big Bang Nucleosynthesis
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Success of the small mass ratio approximation during the final orbits of binary black hole simulations
• Efficiency of nonspinning templates in gravitational wave searches for aligned-spin binary black holes
• Quasinormal Modes by Improved Matrix Method and Weighted Residual Method
• Constraints and prospects on gravitational wave and neutrino emission using GW150914
• Constraining Black Hole Populations in Globular Clusters using Microlensing: Application to Omega Centauri
• Constraints and prospects on GW and neutrino emissions using GW150914
• Search for Coincident Gravitational Wave and Long Gamma-Ray Bursts from 4-OGC and the Fermi-GBM/Swift-BAT Catalog
• A Drop in the Pond: The Effect of Rapid Mass Loss on the Dynamics and Interaction Rate of Collisionless Particles
• Limiting the Number of Extra Dimensions with Shortcuts
• The gravitational Higgs mechanism and resulting smoking gun effects
• Signatures of regular black holes from the quasar continuum spectrum
• A novel multi-layer modular approach for real-time fuzzy-identification of gravitational-wave signals
• Limits on the Electro-Magnetic Counterpart of Binary Black Hole Coalescence at Visible Wavelengths
• On the Gauge Invariance of Secondary Gravitational Waves
• Trumpet Initial Data for Boosted Black Holes
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• Random projections in gravitational wave searches of compact binaries
• A class of regular bouncing cosmologies
• Disentangling the potential dark matter origin of LIGO's black holes
• Implications of binary black hole detections on the merger rates of double neutron stars and neutron star-black holes
• Search for sub-solar mass binaries with Einstein Telescope and Cosmic Explorer
• Testing the Wave-Particle Duality of Gravitational Wave Using the Spin-Orbital-Hall Effect of Structured Light
• Hawking effect in an extremal Kerr black hole spacetime
• Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
• Noncommutative Reissner-Nordström black hole from noncommutative charged scalar field
• Design and experimental demonstration of a laser modulation system for future gravitational-wave detectors
• Inflationary relics from an Ultra-Slow-Roll plateau
• A General Discussion on Photon Spheres in Different Categories of Spacetimes
• Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
• On the Possibility of Direct Detection of the Emission of Microlens MOA-2011-BLG-191/OGLE-2011-BLG-0462 -- a Probable Black Hole
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture framework
• Primordial Black Holes and Second-order Gravitational Waves in Axion-like Hybrid Inflation
• Primary gravitational waves at high frequencies I: Origin of suppression in the power spectrum
• Gravitational radiation from birefringent matter dynamics
• Sky localization of space-based detectors with time-delay interferometry
• Gravitational wave induced baryon acoustic oscillations
• Quantum Oppenheimer-Snyder models in loop quantum cosmology with Lorentz term
• Laser Interferometer in Presence of Scalar field on Gravitational Wave Background
• Looking for ancillary signals around GW150914
• Progenitors of binary black hole mergers detected by LIGO
• A "nu" look at gravitational waves: The black hole birth rate from neutrinos combined with the merger rate from LIGO
• Astrophysical uncertainties challenge 21-cm forecasts: A primordial black hole case study
• Dark Matter and Fundamental Physics Searches with IACTs
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Optimal follow-up observations of gravitational wave events with small optical telescopes
• Mass function of stellar black holes as revealed by the LIGO-Virgo-KAGRA observations
• Constraining black-hole horizon effects by LIGO-Virgo detections of inspiralling binary black holes
• Period-Luminosity-Metallicity-Color Relations of Late-type Contact Binaries in the Big Data Era
• Detecting milli-Hz gravitational waves with optical resonators
• Dynamical friction from scalar dark matter in the relativistic regime
• Implementation of the rROF denoising method in the cWB pipeline for gravitational-wave data analysis
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Hierarchical Merger of Primordial Black Holes in Dwarf Galaxies
• Dynamical environments of relativistic binaries: The phenomenon of resonance shifting
• Constraints on generalized Eddington-inspired Born-Infeld branes
• Brans-Dicke analogue of the Roberts geometry
• Bounding dark charges on binary black holes using gravitational waves
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• Optimizing signal recycling for detecting a stochastic gravitational-wave background
• Pearson cross-correlation in the first four black hole binary mergers
• Effective-one-body formalism for leading-order radiative effects in the post-linear framework
• Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
• Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes
• Aspects of Spatially-Correlated Random Fields: Extreme-Value Statistics and Clustering Properties
• New numerical framework for the generalized Baumgarte-Shapiro-Shibata-Nakamura formulation: The vacuum case for spherical symmetry
• Quasar continuum spectrum disfavors black holes with a magnetic monopole charge
• Bardeen-Kiselev black hole with cosmological constant
• Correlating Gravitational Wave and Gamma-ray Signals from Primordial Black Holes
• Evaluating statistical significance for massive black hole binary mergers with space-based gravitational wave detectors
• Bispectrum of induced gravitational waves in the poltergeist mechanism
• 'Stealth' singularities from self-gravitating fermions
• The Fourth RIT binary black hole simulations catalog: Extension to Eccentric Orbits
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• Global time-frequency search for stellar-mass binary black holes in LISA
• On the ease of excitation of black hole ringing: Quantifying the importance of overtones by the excitation factors
• $\kappa$-General-Relativity II: An Astrophysical Observable from a 2-Body system
• Probing neutron stars with the full pre-merger and post-merger gravitational wave signal from binary coalescences
• Gravitational acceleration in a class of geometric sigma models
• Alternative LISA-TAIJI networks: detectability of the isotropic stochastic gravitational wave background
• Search for sub-solar primordial black holes in low mass ratio binaries with LIGO-Virgo O2 data and implications for the primordial black hole dark matter fraction
• The initial value problem for gravitational waves in conformal gravity