GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

Abstract

On August 14, 2017 at 10:30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm-rate of $\lesssim$ 1 in 27000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are $30.5_{-3.0}^{+5.7}$ Msun and $25.3_{-4.2}^{+2.8}$ Msun (at the 90% credible level). The luminosity distance of the source is $540_{-210}^{+130}\mathrm{Mpc}$, corresponding to a redshift of $z=0.11_{-0.04}^{+0.03}$. A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160 deg${}^2$ using only the two LIGO detectors to 60 deg${}^2$ using all three detectors. For the first time, we can test the nature of gravitational wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling a new class of phenomenological tests of gravity.

References in corpus (101)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• Planck 2015 results. XIII. Cosmological parameters
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• The Confrontation between General Relativity and Experiment
• Advanced LIGO
• GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Tests of general relativity with GW150914
• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Evolution of Binary Black Hole Spacetimes
• Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision
• Effective one-body approach to general relativistic two-body dynamics
• Gravitational wave extraction from an inspiraling configuration of merging black holes
• LIGO: The Laser Interferometer Gravitational-Wave Observatory
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
• Properties of the Binary Black Hole Merger GW150914
• Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
• Transition from inspiral to plunge in binary black hole coalescences
• Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
• Using gravitational-wave standard sirens
• GW150914: The Advanced LIGO Detectors in the Era of First Discoveries
• Observing binary inspiral in gravitational radiation: One interferometer
• A simple model of complete precessing black-hole-binary gravitational waveforms
• The PyCBC search for gravitational waves from compact binary coalescence
• FINDCHIRP: an algorithm for detection of gravitational waves from inspiraling compact binaries
• Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
• Timing Measurements of the Relativistic Binary Pulsar PSR B1913+16
• Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian order
• Search templates for gravitational waves from inspiraling binaries: Choice of template spacing
• The Sensitivity of the Advanced LIGO Detectors at the Beginning of Gravitational Wave Astronomy
• Effective-one-body model for black-hole binaries with generic mass ratios and spins
• Matched filtering of gravitational waves from inspiraling compact binaries: Computational cost and template placement
• Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
• BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
• Testing General Relativity with Pulsar Timing
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
• Rapid Bayesian position reconstruction for gravitational-wave transients
• The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914
• Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order
• Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
• Localization and broadband follow-up of the gravitational-wave transient GW150914
• Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
• BayesLine: Bayesian Inference for Spectral Estimation of Gravitational Wave Detector Noise
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence
• Toward Early-Warning Detection of Gravitational Waves from Compact Binary Coalescence
• Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope
• The final spin from binary black holes in quasi-circular orbits
• An improved analytical description of inspiralling and coalescing black-hole binaries
• Model-Independent Test of General Relativity: An Extended post-Einsteinian Framework with Complete Polarization Content
• Implementing a search for aligned-spin neutron star -- black hole systems with advanced ground based gravitational wave detectors
• An improved effective-one-body Hamiltonian for spinning black-hole binaries
• Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up
• Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
• Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy
• The First Two Years of Electromagnetic Follow-Up with Advanced LIGO and Virgo
• Triangulation of gravitational wave sources with a network of detectors
• Fast and Accurate Inference on Gravitational Waves from Precessing Compact Binaries
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
• Source localization with an advanced gravitational wave detector network
• An improved analysis of GW150914 using a fully spin-precessing waveform model
• Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
• A stochastic template placement algorithm for gravitational wave data analysis
• Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era
• High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube
• Detecting binary neutron star systems with spin in advanced gravitational-wave detectors
• Effects of waveform model systematics on the interpretation of GW150914
• Multi-timescale analysis of phase transitions in precessing black-hole binaries
• A novel scheme for rapid parallel parameter estimation of gravitational waves from compact binary coalescences
• A data-analysis strategy for detecting gravitational-wave signals from inspiraling compact binaries with a network of laser-interferometric detectors
• GEO 600 and the GEO-HF upgrade program: successes and challenges
• Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914
• Remnant of binary black-hole mergers: New simulations and peak luminosity studies
• An effectual template bank for the detection of gravitational waves from inspiralling compact binaries with generic spins
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Calibration and sensitivity of the Virgo detector during its second science run
• Probing Dynamical Gravity with the Polarization of Continuous Gravitational Waves
• Estimating the parameters of non-spinning binary black holes using ground-based gravitational-wave detectors: Statistical errors
• Mechanical loss in state-of-the-art amorphous optical coatings
• The Advanced LIGO Photon Calibrators
• Modeling the source of GW150914 with targeted numerical-relativity simulations
• Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914
• Environmental Influences on the LIGO Gravitational Wave Detectors during the 6th Science Run
• Comparison of Gravitational Wave Detector Network Sky Localization Approximations
• Supplement: Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up
• On Discovering Electromagnetic Emission from Neutron Star Mergers: The Early Years of Two Gravitational Wave Detectors
• Active noise cancellation in a suspended interferometer
• Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Regression of Environmental Noise in LIGO Data
• Measuring intermediate mass black hole binaries with advanced gravitational wave detectors
• The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity
• Increasing LIGO sensitivity by feedforward subtraction of auxiliary length control noise
• Finding the One: Identifying the Host Galaxies of Gravitational-Wave Sources
• Estimating parameters of binary black holes from gravitational-wave observations of their inspiral, merger and ringdown
• Where angular momentum goes in a precessing black hole binary
• Reconstruction of the gravitational wave signal $h(t)$ during the Virgo science runs and independent validation with a photon calibrator

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• A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity
• Dynamics of compact binary systems in scalar-tensor theories: I. Equations of motion to the third post-Newtonian order
• Binary Black Hole Mergers from Globular Clusters: the Impact of Globular Cluster Properties
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• Dynamics of black hole - neutron star binaries in young star clusters
• An Analytical Portrait of Binary Mergers in Hierarchical Triple Systems
• What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses
• Shadows of Kerr-like black holes in a modified gravity theory
• Constraining the primordial black hole abundance with 21cm cosmology
• Science with the TianQin observatory: Preliminary results on testing the no-hair theorem with ringdown signals
• A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey
• Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run
• Polarizations of Gravitational Waves in Horndeski Theory
• Head-on collisions and orbital mergers of Proca stars
• A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity
• Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds
• The MEGaN project II. Gravitational waves from intermediate mass- and binary black holes around a supermassive black hole
• Gravitational Waves from Binary Mergers of Sub-solar Mass Dark Black Holes
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• Quasi-normal modes of black holes in Horndeski gravity
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• Decoding the phases of early and late time reheating through imprints on primordial gravitational waves
• Gravitational-Wave Emission from Binary Black Holes Formed in Open Clusters
• Effects of the surrounding primordial black holes on the merger rate of primordial black hole binaries
• Constraining the Inclination of Binary Mergers from Gravitational-wave Observations
• Searches for Continuous Gravitational Waves from Fifteen Supernova Remnants and Fomalhaut b with Advanced LIGO
• Hidden universality in the merger rate distribution in the primordial black hole scenario
• 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
• Relaxations of perturbations of spacetimes in general relativity coupled to nonlinear electrodynamics
• Neutrino transport in black hole-neutron star binaries: neutrino emission and dynamical mass ejection
• Chaotic shadow of a non-Kerr rotating compact object with quadrupole mass moment
• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Screw-symmetric gravitational waves: a double copy of the vortex
• Constraints on scalar-tensor theory of gravity by the recent observational results on gravitational waves
• Noise spectral estimation methods and their impact on gravitational wave measurement of compact binary mergers
• Black-hole ringdown as a probe of higher-curvature gravity theories
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Accelerating black holes: quasinormal modes and late-time tails
• Template-based Gravitational-Wave Echoes Search Using Bayesian Model Selection
• Rush the inspiral: efficient Effective One Body time-domain gravitational waveforms
• Numerical Relativity of Compact Binaries in the 21st Century
• Time-Delay Interferometry and Clock-Noise Calibration
• 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
• The peculiar acceleration of stellar-origin black hole binaries: measurement and biases with LISA
• Detection and Classification of Supernova Gravitational Waves Signals: A Deep Learning Approach
• Intrinsic curvature and topology of shadows in Kerr spacetime
• EHT tests of the strong-field regime of General Relativity
• Testing the nature of gravitational-wave polarizations using strongly lensed signals
• 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
• On the gauge dependence of gravitational waves generated at second order from scalar perturbations
• Fourier domain gravitational waveforms for precessing eccentric binaries
• A hybrid post-Newtonian -- effective-one-body scheme for spin-precessing compact-binary waveforms
• SENR/NRPy+: Numerical Relativity in Singular Curvilinear Coordinate Systems
• Eikonal quasinormal modes of black holes beyond General Relativity
• Effective stability against superradiance of Kerr black holes with synchronised hair
• Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation
• Observatory science with eXTP
• A New Method to Observe Gravitational Waves emitted by Core Collapse Supernovae
• Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• Overcoming the SQL in gravitational wave detectors using spin systems with negative effective mass
• The effects of surface fossil magnetic fields on massive star evolution: I. Magnetic field evolution, mass-loss quenching and magnetic braking
• Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
• Probing the Lorentz Symmetry Violation Using the First Image of Sagittarius A*: Constraints on Standard-Model Extension Coefficients
• Gravitational waves from compact binaries in post-Newtonian accurate hyperbolic orbits
• Accelerating parameter inference with graphics processing units
• Black Hole and Neutron Star Binary Mergers in Triple Systems: II. Merger Eccentricity and Spin-Orbit Misalignment
• On the Ambiguity in Relativistic Tidal Deformability
• Neutron Star Mergers and How to Study Them
• Prospects for detecting gravitational waves at 5 Hz with ground-based detectors
• Constraining f(R) gravity in solar system, cosmology and binary pulsar systems
• Small-scale structure of primordial black hole dark matter and its implications for accretion
• Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
• Velocity Memory Effect for Polarized Gravitational Waves
• Populations of stellar mass Black holes from binary systems
• Black Hole Echology: The Observer's Manual
• Polarizations of Gravitational Waves in the Bumblebee Gravity Model
• A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
• Effects of the merger history on the merger rate density of primordial black hole binaries
• Stellar Black Hole Binary Mergers in Open Clusters
• The Formation of Intermediate Mass Black Holes in Galactic Nuclei
• Detecting Supermassive Black Hole-Induced Binary Eccentricity Oscillations with LISA
• Spectral separation of the stochastic gravitational-wave background for LISA: observing both cosmological and astrophysical backgrounds
• Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-Wave Detections
• Relativistic stars in vector-tensor theories
• Applying deep neural networks to the detection and space parameter estimation of compact binary coalescence with a network of gravitational wave detectors
• Gravitational Waves from Dark Boson Star binary mergers
• Single-single gravitational-wave captures in globular clusters: Eccentric deci-Hertz sources observable by DECIGO and Tian-Qin
• Constraining black hole mimickers with gravitational wave observations
• Merger rate density of binary black holes formed in open clusters
• Anisotropies in the astrophysical gravitational-wave background: The impact of black hole distributions
• The merger history of primordial-black-hole binaries
• Observational tests of the black hole area increase law
• Stellar binary black holes in the LISA band: a new class of standard sirens
• Gravitational wave energy emission and detection rates of Primordial Black Hole hyperbolic encounters
• Propagation of gravitational waves in teleparallel gravity theories
• Parameter estimation for black hole echo signals and their statistical significance
• Polarization test of gravitational waves from compact binary coalescences
• Oscillation modes of hybrid stars within the relativistic Cowling approximation
• Parameter Estimation with a spinning multi-mode waveform model: IMRPhenomHM
• Quasinormal Modes of Modified Gravity (MOG) Black Holes
• Turbulence of Weak Gravitational Waves in the Early Universe
• Gravitational Waves in $F(R)$ Gravity: Scalar Waves and the Chameleon Mechanism
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Radiation reaction for spinning black-hole scattering
• Propagation of the gravitational waves in a cosmological background
• Hyperspectral Pixel Unmixing with Latent Dirichlet Variational Autoencoder
• Probing planetary-mass primordial black holes with continuous gravitational waves
• Hairy binary black holes in Einstein-Maxwell-dilaton theory and their effective-one-body description
• Measuring the eccentricity of GW170817 and GW190425
• Characterising Transient Noise in the LIGO Detectors
• On the dynamical bar-mode instability in spinning bosonic stars
• Modeling ringdown II: non-precessing binary black holes
• Tracking black hole kicks from gravitational wave observations
• Formation of primordial black holes in an axionlike curvaton model
• Black Hole Pulsar
• Parameter Estimation and Model Selection of Gravitational Wave Signals Contaminated by Transient Detector Noise Glitches
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• A correspondence between modified gravity and General Relativity with scalar fields
• Spontaneous scalarization of charged black holes at the approach to extremality
• Can we distinguish low mass black holes in neutron star binaries?
• Virgo Detector Characterization and Data Quality: results from the O3 run
• Exciting black hole modes via misaligned coalescences: I. Inspiral, transition, and plunge trajectories using a generalized Ori-Thorne procedure
• Primordial black holes and secondary gravitational waves from natural inflation
• A self-consistent method to estimate the rate of compact binary coalescences with a Poisson mixture model
• Waveform of gravitational waves in the ghost-free parity-violating gravities
• Dynamical formation of Proca stars and quasi-stationary solitonic objects
• Effectual gravitational-wave template banks for coalescing compact binaries using a hybrid placement algorithm
• Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2
• Massively Parallel Simulations of Binary Black Hole Intermediate-Mass-Ratio Inspirals
• The formation rate of short gamma-ray bursts and gravitational waves
• Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections
• Probing Gravitational Parity Violation with Gravitational Waves from Stellar-mass Black Hole Binaries
• General theories of linear gravitational perturbations to a Schwarzschild Black Hole
• The signal of the stochastic gravitational wave background and the angular correlation of its energy density
• Features of the inflaton potential and the power spectrum of cosmological perturbations
• Quantum sensor networks as exotic field telescopes for multi-messenger astronomy
• Constraining black-hole spins with gravitational wave observations
• Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing run
• Unraveling the origin of black holes from effective spin measurements with LIGO-Virgo
• Unified model for the LISA measurements and instrument simulations
• Detecting the anisotropic astrophysical gravitational wave background in the presence of shot noise through cross-correlations
• New rotating black holes in non-linear Maxwell $f(\mathcal{R})$ gravity
• Constraining the Polarization Content of Gravitational Waves with Astrometry
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• Constraining alternative theories of gravity using pulsar timing arrays
• New class of quasinormal modes of neutron stars in scalar-tensor gravity
• Dependence of outer boundary condition on protoneutron star asteroseismology with gravitational-wave signatures
• Gravitational wave signatures of dark matter cores in binary neutron star mergers by using numerical simulations
• Assessing the impact of transient orbital resonances
• Confronting Models of Massive Star Evolution and Explosions with Remnant Mass Measurements
• Order in the chaos: eccentric black hole binary mergers in triples formed via strong binary-binary scatterings
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation III: dissecting black hole dynamics
• Testing the multipole structure of compact binaries using gravitational wave observations
• Angular momentum transport in massive stars and natal neutron star rotation rates
• Primordial black holes and scalar induced gravitational waves from the $E$ model with a Gauss-Bonnet term
• Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Mapping dynamical ejecta and disk masses from numerical relativity simulations of neutron star mergers
• Primordial black holes and secondary gravitational waves from the Higgs field
• Damping of gravitational waves by matter
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems
• Generic searches for alternative gravitational wave polarizations with networks of interferometric detectors
• Black Hole Formation in Fallback Supernova and the Spins of LIGO Sources
• A "no-hair" test for binary black holes
• Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities
• Designing Horndeski and the effective fluid approach
• Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
• Irreducible background of gravitational waves from a cosmic defect network: update and comparison of numerical techniques
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone
• Spectral classification of gravitational-wave emission and equation of state constraints in binary neutron star mergers
• The Polarizations of Gravitational Waves
• Shadows of charged rotating black holes: Kerr-Newman versus Kerr-Sen
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Tail contributions and post-adiabatic corrections
• Gravitational wave constraints on Lorentz and parity violations in gravity: high-order spatial derivative cases
• Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
• Innermost stable circular orbit of spinning particle in charged spinning black hole background
• Picometer-stable hexagonal optical bench to verify LISA phase extraction linearity and precision
• Topological Stars, Black holes and Generalized Charged Weyl Solutions
• Primordial black holes and induced gravitational waves in $k$-inflation
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• Reconstruction of Power Spectrum of Primordial Curvature Perturbations on small scales from Primordial Black Hole Binaries scenario of LIGO/VIRGO detection
• Constraints on the Nieh-Yan modified teleparallel gravity with gravitational waves
• Mass and spin of a Kerr black hole in modified gravity and a test of the Kerr black hole hypothesis
• A new data analysis framework for the search of continuous gravitational wave signals
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions
• Impact of infrasound atmospheric noise on gravity detectors used for astrophysical and geophysical applications
• The hangup effect in unequal mass binary black hole mergers and further studies of their gravitational radiation and remnant properties
• Binary Pulsar constraints on massless scalar-tensor theories using Bayesian statistics
• On the motion of hairy black holes in Einstein-Maxwell-dilaton theories
• Neutral regular black hole solution in generalized Rastall gravity
• Ready-to-use Fourier domain templates for compact binaries inspiraling along moderately eccentric orbits
• The host galaxies of double compact objects merging in the local Universe
• Non-polynomial Lagrangian approach to Regular Black Holes
• Evolution of Galaxy Star Formation and Metallicity: Impact on Double Compact Objects Mergers
• Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity
• A Simflowny-based finite-difference code for high-performance computing in Relativity
• Testing General Relativity with Gravitational Waves: An Overview
• Classifying the unknown: discovering novel gravitational-wave detector glitches using similarity learning
• Hunting for the host galaxy groups of binary black holes and the application in constraining Hubble constant
• Axion star collisions with black holes and neutron stars in full 3D numerical relativity
• Quasi-normal mode frequencies and gravitational perturbations of black holes with any subextremal spin in modified gravity through METRICS: the scalar-Gauss-Bonnet gravity case
• Polarized image of a Schwarzschild black hole with a thin accretion disk as photon couples to Weyl tensor
• Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
• Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise
• Binary neutron star mergers: Effects of spin and post-merger dynamics
• Primordial black holes and gravitational waves in nonstandard cosmologies
• Absorption, Scattering, Geodesics, Shadows and Lensing Phenomena of Black Holes in Effective Quantum Gravity
• Challenges testing the no-hair theorem with gravitational waves
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Constraints on primordial curvature spectrum from primordial black holes and scalar-induced gravitational waves
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies
• Shadows of Exact Binary Black Holes
• Hamiltonians and canonical coordinates for spinning particles in curved space-time
• Accumulating errors in tests of general relativity with gravitational waves: overlapping signals and inaccurate waveforms
• Quasinormal modes of massive scalar fields in four-dimensional wormholes: anomalous decay rate
• Scalar Hairy Black Holes in Four Dimensions are Unstable
• Standard-siren cosmology using gravitational waves from binary black holes
• A method to search for long duration gravitational wave transients from isolated neutron stars using the generalized FrequencyHough
• The LISA-Taiji network: precision localization of massive black hole binaries
• Pure polarization test of GW170814 and GW170817 using waveforms consistent with modified theories of gravity
• Some Optimizations on Detecting Gravitational Wave Using Convolutional Neural Network
• Polarization of a stochastic gravitational wave background through diffusion by massive structures
• Gravitational waves and the polarizations in Hořava gravity after GW170817
• Primordial black holes and scalar-induced gravitational waves from the generalized Brans-Dicke theory
• Small scale induced gravitational waves from primordial black holes, a stringent lower mass bound, and the imprints of an early matter to radiation transition
• Physics of eccentric binary black hole mergers: A numerical relativity perspective
• Tests of general relativity using multiband observations of intermediate mass binary black hole mergers
• Eikonal black hole ringings in generalized energy-momentum squared gravity
• Accretion-induced spin-wandering effects on the neutron star in Scorpius X-1: Implications for continuous gravitational wave searches
• Gravitational radiation from compact binary systems in Einstein-Maxwell-dilaton theories
• $f(R,T)=f(R)+\lambda T$ gravity models as alternatives to cosmic acceleration
• PhaseTracer: tracing cosmological phases and calculating transition properties
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Primordial Black Holes from No-Scale Supergravity
• Evolution of Highly Eccentric Binary Neutron Stars Including Tidal Effects
• Can black hole superradiance be induced by galactic plasmas?
• Primordial Black Hole Dark Matter and LIGO/Virgo Merger Rate from Inflation with Running Spectral Indices: Formation in the Matter- and/or Radiation-Dominated Universe
• Hidden-Sector Modifications to Gravitational Waves From Binary Inspirals
• Gravitational Wave Interference via Gravitational Lensing: Measurements of Luminosity Distance, Lens Mass, and Cosmological Parameters
• Prospects of detecting the nonlinear gravitational wave memory
• Gravitational perturbations of non-singular black holes in conformal gravity
• Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering
• Implications of the NANOGrav result on primordial gravitational waves in nonstandard cosmologies
• Subluminal stochastic gravitational waves in pulsar-timing arrays and astrometry
• The star clusters that make black hole binaries across cosmic time
• Detection of Gravitational Waves Using Bayesian Neural Networks
• Gravitational-Wave Signatures from Compact Object Binaries in the Galactic Center
• Ultra-compact X-ray binaries with He star companions
• A Fermi Gamma-ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-Wave Candidates in Advanced LIGO's First Observing Run
• Quasinormal Modes of a Black Hole with Quadrupole Moment
• Impact of the wave-like nature of Proca stars on their gravitational-wave emission
• Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes
• Alternative LISA-TAIJI networks
• Parameter estimation of stellar-mass black hole binaries with LISA
• Waveforms of compact binary inspiral gravitational radiation in screened modified gravity
• Constraints on the binary black hole nature of GW151226 and GW170608 from the measurement of spin-induced quadrupole moments
• Factorization and resummation: A new paradigm to improve gravitational wave amplitudes. II: the higher multipolar modes
• Sensitivity of gravitational wave searches to the full signal of intermediate mass black hole binaries during the LIGO O1 Science Run
• Primordial black holes and secondary gravitational waves from chaotic inflation
• 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
• Template Bank for Compact Binary Coalescence Searches in Gravitational Wave Data: A General Geometric Placement Algorithm
• Massive and charged scalar field in Kerr-Newman spacetime: Absorption and superradiance
• Frequency response of space-based interferometric gravitational-wave detectors
• Digging the population of compact binary mergers out of the noise
• Identifying when Precession can be Measured in Gravitational Waveforms
• Constraining the parameters of GW150914 & GW170104 with numerical relativity surrogates
• Afterglows and Kilonovae Associated with Nearby Low-Luminosity Short-Duration Gamma-Ray Bursts: Application to GW170817/GRB170817A
• Implications of dedicated seismometer measurements on Newtonian-noise cancellation for Advanced LIGO
• Analog Schwarzschild black holes of Bose-Einstein condensates in a cavity: Quasinormal modes and quasibound states
• Astrometric Effects of Gravitational Wave Backgrounds with non-Einsteinian Polarizations
• Quasinormal modes of weakly charged Einstein-Maxwell-dilaton black holes
• Primordial Black Holes from QCD Axion Bubbles
• Dirichlet Process Gaussian-mixture model: An application to localizing coalescing binary neutron stars with gravitational-wave observations
• Moduli Stars
• Quasinormal modes of compact objects in alternative theories of gravity
• Tests of general relativity with stellar-mass black hole binaries observed by LISA
• Detecting the Stochastic Gravitational Wave Background from Primordial Black Hole Formation
• Observation of squeezed light in the 2 $\mu \mathrm{m}$ region
• Continuous gravitational wave from magnetized white dwarfs and neutron stars: possible missions for LISA, DECIGO, BBO, ET detectors
• The Star Formation History of the Milky Way's Nuclear Star Cluster
• The modification of photon trapping orbits as a diagnostic of non-Kerr spacetimes
• Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube
• Spin-induced deformations and tests of binary black hole nature using third-generation detectors
• Parametrized tests of post-Newtonian theory using principal component analysis
• Gravitational lensing by a black hole in effective loop quantum gravity
• Constraining chameleon field driven warm inflation with Planck 2018 data
• Can we probe Planckian corrections at the horizon scale with gravitational waves?
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Using Deep Learning to Localize Gravitational Wave Sources
• On matrix method for black hole quasinormal modes
• Constraints on Horndeski Theory Using the Observations of Nordtvedt Effect, Shapiro Time Delay and Binary Pulsars
• Reconstruction of Primordial Power Spectrum of curvature perturbation from the merger rate of Primordial Black Hole Binaries
• Bayesian nonparametric spectral density estimation using B-spline priors
• Improved limits on a stochastic gravitational-wave background and its anisotropies from Advanced LIGO O1 and O2 runs
• Cosmological inference from standard sirens without redshift measurements
• New Exact Spherically Symmetric Solutions in $f(R,\varphi ,X)$ gravity by Noether's symmetry approach
• A static and spherically symmetric hairy black hole in the framework of the Gravitational Decoupling
• Bayesian Metric Reconstruction with Gravitational Wave Observations
• The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814
• Primordial black holes and secondary gravitational waves from string inspired general no-scale supergravity
• Quasinormal spectra of scale-dependent Schwarzschild-de Sitter black holes
• Second post-Newtonian order radiative dynamics of inspiralling compact binaries in the Effective Field Theory approach
• Very fast stochastic gravitational wave background map making using folded data
• Mechanisms of Producing Primordial Black Holes By Breaking The SU(2,1)/SU(2)$\times$U(1) Symmetry
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Non-Minimal Einstein-Yang-Mills Black Holes: Fundamental Quasinormal Mode and Grey-Body factors versus Outburst of Overtones
• Viewing angle of binary neutron star mergers
• Chaotic Shadows of Black Holes: A Short Review
• Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
• Gravitational Waves and Primordial Black Holes from Supersymmetric Hybrid Inflation
• How well can ultracompact bodies imitate black hole ringdowns?
• Black hole spins in coalescing binary black holes
• Comparison of various methods to extract ringdown frequency from gravitational wave data
• NANOGrav signal and LIGO-Virgo Primordial Black Holes from the Higgs field
• Primordial black holes and gravitational waves from nonminimally coupled supergravity inflation
• Numerical relativity in spherical coordinates: A new dynamical spacetime and general relativistic MHD evolution framework for the Einstein Toolkit
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• The Eccentric Behavior of Inspiraling Compact Binaries
• Fusing numerical relativity and deep learning to detect higher-order multipole waveforms from eccentric binary black hole mergers
• Primordial black holes ensued from exponential potential and coupling parameter in nonminimal derivative inflation model
• Localization of binary mergers with gravitational-wave detectors of second and third generation
• Quasinormal modes of an improved Schwarzschild black hole
• Primordial gravitational waves in Horndeski gravity
• DDF operators, open string coherent states and their scattering amplitudes
• Characterisation of lensing selection effects for LISA massive black hole binary mergers
• Spectral method for metric perturbations of black holes: Kerr background case in general relativity
• High-power all-fiber ultra-low noise laser
• Implementing a semicoherent search for continuous gravitational waves using optimally-constructed template banks
• Merger estimates for rotating Kerr black holes in modified gravity
• Fundamental Symmetries and Spacetime Geometries in Gauge Theories of Gravity: Prospects for Unified Field Theories
• A wider look at the gravitational-wave transients from GWTC-1 using an unmodeled reconstruction method
• Multimessenger tests of the weak equivalence principle from GW170817 and its electromagnetic counterparts
• Populating the Black Hole Mass Gaps In Stellar Clusters: General Relations and Upper Limits
• Gravitational redshift/blueshift of light emitted by geodesic test particles, frame-dragging and pericentre-shift effects, in the Kerr-Newman-de Sitter and Kerr-Newman black hole geometries
• Simple procedures to reduce eccentricity of binary black hole simulations
• Probing gravitational wave polarizations with Advanced LIGO, Advanced Virgo and KAGRA
• Searching for anisotropy in the distribution of binary black hole mergers
• $F(R)$ Gravity with an Axion-like Particle: Dynamics, Gravity Waves, Late and Early-time Phenomenology
• Spectral Method for the Gravitational Perturbations of Black Holes: Schwarzschild Background Case
• Shadows of rotating Hayward-de Sitter black holes with astrometric observables
• NuRIA: Numerical Relativity Injection Analysis of spinning binary black hole signals in Advanced LIGO data
• Determination of properties of protoneutron stars toward black hole formation via gravitational wave observations
• X-ray Detectability of Accreting Isolated Black Holes in Our Galaxy
• All-sky search for long-duration gravitational-wave transients in the second Advanced LIGO observing run
• Strong-lensing of Gravitational Waves by Galaxy Clusters
• Gravitational Lensing of Gravitational Waves: Rotation of Polarization Plane
• Deep and rapid observations of strong-lensing galaxy clusters within the sky localisation of GW170814
• The Maximal-Density Mass Function for Primordial Black Hole Dark Matter
• Ringing of a black hole in a dark matter halo
• Sensitivity functions for space-borne gravitational wave detectors
• Echoes of Compact Objects in Scalar-Tensor Theories of Gravity
• Primordial black holes in non-canonical scalar field inflation driven by quartic potential in the presence of bump
• The Effect of Distant Encounters on Black Hole Binaries in Globular Clusters: Systematic Increase of In-cluster Mergers in the LISA band
• Neutron Star-Black Hole Mergers from Gravitational Wave Captures
• Intensity and anisotropies of the stochastic Gravitational Wave background from merging compact binaries in galaxies
• A 6D interferometric inertial isolation system
• Gravitational Waves in f(R) Gravity Power Law Model
• The host galaxies of double compact objects across cosmic time
• Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory
• All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run
• Methods for the detection of gravitational waves from sub-solar mass ultracompact binaries
• Gravitational waves in Einstein-Æther theory and generalized TeVeS theory after GW170817
• Black hole perturbations in vector-tensor theories: The odd-mode analysis
• Gauge transformation of scalar induced gravitational waves
• Ultra long lived quasinormal modes of neutron stars in massive scalar-tensor gravity
• Theory-agnostic Reconstruction of Potential and Couplings from Quasi-Normal Modes
• Neutron star collapse and gravitational waves with a non-convex equation of state
• Numerical simulation of time delay interferometry for new LISA, TAIJI and other LISA-like missions
• A new approach and code for spinning black holes in modified gravity
• Forming Pop III binaries in self-gravitating disks: how to keep the orbital angular momentum
• On the Potential Observation of False Deviations from General Relativity in Gravitational Wave Observations from Binary Black Holes
• A Single Progenitor Model for GW150914 and GW170104
• Tidal Love numbers of Proca stars
• Reconstructing gravitational wave signals from binary black hole mergers with minimal assumptions
• 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
• Cosmography with next-generation gravitational wave detectors
• Measuring stochastic gravitational-wave energy beyond general relativity
• Absorption of electromagnetic plane waves by rotating black holes
• Compact object mergers driven by gas fallback
• Refined clock-jitter reduction in the Sagnac-type time-delay interferometry combinations
• Probing cosmological fields with gravitational wave oscillations
• Common-envelope Dynamics of a Stellar-mass Black Hole: General Relativistic Simulations
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Gravitational waves and extra dimensions: a short review
• Gravitational waves in massive gravity theories: waveforms, fluxes and constraints from extreme-mass-ratio mergers
• Double Gravitational Wave Mergers
• Theoretical and observational constraints on regularized 4$D$ Einstein-Gauss-Bonnet gravity
• Full distribution of clusters with universal couplings and in-medium effects
• Lensing of Gravitational Waves as a Novel Probe of Graviton Mass
• First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics
• Gauge transformation of scalar induced tensor perturbation during matter domination
• Numerical relativity in spherical coordinates with the Einstein Toolkit
• On Thermal Stability of Hairy Black Holes
• Effects of non-commutative geometry on black hole properties
• Comparison of binary black hole initial data sets
• Search for gravitational waves from five low mass X-ray binaries in the second Advanced LIGO observing run with an improved hidden Markov model
• Laser Frequency Noise in Next Generation Gravitational-Wave Detectors
• I-Love-Q Relations for Neutron Stars in dynamical Chern Simons Gravity
• Compact multi-fringe interferometry with sub-picometer precision
• On the propagation of gravitational waves in strong magnetic fields
• How loud are echoes from exotic compact objects?
• Binary Neutron Stars Gravitational Wave Detection Based on Wavelet Packet Analysis And Convolutional Neural Networks
• Investigating the relation between gravitational wave tests of general relativity
• Anomaly Detection in Gravitational Waves data using Convolutional AutoEncoders
• A Linear and Quadratic Time-Frequency Analysis of Gravitational Waves from Core-Collapse Supernovae
• Circular polarization of gravitational waves from non-rotating supernova cores: a new probe into the pre-explosion hydrodynamics
• Quasinormal modes of dilatonic Reissner-Nordström black holes
• Gravitational-wave merging events from the dynamics of stellar mass binary black holes around the massive black hole in a galactic nucleus
• Assessing the Energetics of Spinning Binary Black Hole Systems
• Prospects for gravitational-wave polarization test from compact binary mergers with future ground-based detectors
• On networks of space-based gravitational-wave detectors
• Towards a framework for testing general relativity with extreme-mass-ratio-inspiral observations
• Absorption by black hole remnants in metric-affine gravity
• Primordial Black Holes as Dark Matter: Constraints From Compact Ultra-Faint Dwarfs
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• Constraints from the Time Lag between Gravitational Waves and Gamma Rays: Implications of GW 170817 and GRB 170817A
• Spectral Cauchy-characteristic extraction of the gravitational wave news function
• Targeted numerical simulations of binary black holes for GW170104
• Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
• Measuring the Speed of Gravitational Waves from the First and Second Observing Run of Advanced LIGO and Advanced Virgo
• Full analytical formulas for frequency response of space-based gravitational wave detectors
• On gravastar formation: What can be the evidence of a black hole?
• Binary White Dwarfs as Laboratories for Extreme Gravity with LISA
• Kinematic signatures of reverberation mapping of close binaries of supermassive black holes in active galactic nuclei
• Electromagnetic precursor flares from the late inspiral of neutron star binaries
• Systematic challenges for future gravitational wave measurements of precessing binary black holes
• Enhancing confidence in the detection of gravitational waves from compact binaries using signal coherence
• Observing gravitational wave polarizations with LISA-TAIJI network
• Parametrizing gravitational-wave polarizations
• The formation of single neutron-stars from double white-dwarf mergers via accretion-induced collapse
• Axial quasinormal modes of static neutron stars in the nonminimal derivative coupling sector of Horndeski gravity: spectrum and universal relations for realistic equations of state
• A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
• Improving significance of binary black hole mergers in Advanced LIGO data using deep learning : Confirmation of GW151216
• Binary neutron star merger rate via the luminosity function of short gamma-ray bursts
• Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• CMB spectral distortions from black holes formed by vacuum bubbles
• An astrophysically motivated ranking criterion for low-latency electromagnetic follow-up of gravitational wave events
• Eccentric Mergers in AGN Discs: Influence of the Supermassive Black-Hole on Three-body Interactions
• Data-driven spectroscopic estimates of absolute magnitude, distance and binarity -- method and catalog of 16,002 O- and B-type stars from LAMOST
• Black hole Spin Measurement Based on Time-domain VLBI Observations of Infalling Gas Cloud
• Characterization of binary black holes by heterogeneous gravitational-wave networks
• Supernova explosions of massive stars and cosmic rays
• Using negative-latency gravitational wave alerts to detect prompt radio bursts from binary neutron star mergers with the Murchison Widefield Array
• Gravitational waves from spinning binary black holes at the leading post-Newtonian orders at all orders in spin
• Repeated faint quasinormal bursts in extreme-mass-ratio inspiral waveforms: Evidence from frequency-domain scalar self-force calculations on generic Kerr orbits
• Total-variation methods for gravitational-wave denoising: performance tests on Advanced LIGO data
• Topological approach to derive the global Hawking temperature of (massive) BTZ black hole
• Sky localization of space-based gravitational wave detectors
• Atomic Interferometric Gravitational-wave Space Observatory (AIGSO)
• Electromagnetic Chirps from Neutron Star-Black Hole Mergers
• A robust machine learning algorithm to search for continuous gravitational waves
• Searching for Cross-Correlation Between Stochastic Gravitational Wave Background and Galaxy Number Counts
• The perturbative approach for the weak deflection angle
• Scalar-tensor mixed polarization search of gravitational waves
• Exploring non-singular black holes in gravitational perturbations
• Full 3D Numerical Relativity Simulations of Neutron Star -- Boson Star Collisions with BAM
• Exact Black Hole Solutions in Modified Gravity Theories: Spherical Symmetry Case
• Limits on primordial magnetic fields from direct detection experiments of gravitational wave background
• Image of Bonnor black dihole with a thin accretion disk and its polarization information
• Primordial black holes formation and secondary gravitational waves in nonminimal derivative coupling inflation
• NANOGrav Hints on Planet-Mass Primordial Black Holes
• Sharp turns in axion monodromy: primordial black holes and gravitational waves
• How does the Earth's rotation affect predictions of gravitational wave strong lensing rates?
• Frequency response of time-delay interferometry for space-based gravitational wave antennas
• Simulating Transient Noise Bursts in LIGO with Generative Adversarial Networks
• Exploring stellar evolution with gravitational-wave observations
• Echoes from a singularity
• Geometric approach for the modified second generation time delay interferometry
• The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
• Charged Black Hole Mergers: Orbit Circularisation and Chirp Mass Bias
• Black Hole Ringdown as a Probe for Dark Energy
• Spectral Lines of Quantized, Spinning Black Holes and their Astrophysical Relevance
• New self-consistent effective one-body theory for spinless binaries based on the post-Minkowskian approximation
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• Magnetized accretion disks around Kerr black holes with scalar hair - I. Constant angular momentum disks
• CG X-1: an eclipsing Wolf-Rayet ULX in the Circinus galaxy
• Constraining alternative polarization states of gravitational waves from individual black hole binaries using pulsar timing arrays
• The Population of Eccentric Binary Black Holes: Implications for mHz Gravitational Wave Experiments
• Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
• Gravitational wave constraints on spatial covariant gravities
• The Advanced Virgo Photon Calibrators
• Rotating black holes in Eddington-inspired Born-Infeld gravity: an exact solution
• Correlated magnetic noise from anisotropic lightning sources and the detection of stochastic gravitational waves
• Moment of inertia - mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
• Eccentricity distributions of eccentric binary black holes in galactic nuclei
• Gravitational Wave Background Sky Maps from Advanced LIGO O1 Data
• Constraining Compact Object Formation with 2M0521
• Testing General Relativity with Black Hole-Pulsar Binaries
• First Tests of a Newtonian Calibrator on an Interferometric Gravitational Wave Detector
• Finslerian Ressiner-Nordstrom spacetime
• A more stringent constraint on the mass ratio of binary neutron star merger GW170817
• dart_board: Binary Population Synthesis with Markov Chain Monte Carlo
• Astrometric Effects of Gravitational Wave Backgrounds with non-Luminal Propagation Speeds
• Self-consistent Effective-one-body theory for spinless binaries based on post-Minkowskian approximation I: Hamiltonian and decoupled equation for ${\psi }_4^B$
• Stability of black holes with non-minimally coupled scalar hair to the Einstein tensor
• Axial quasi-normal modes of neutron stars in $R^2$ gravity
• Population III star formation in an X-ray background: III. Periodic radiative feedback and luminosity induced by elliptical orbits
• Kerr-(Anti-)de Sitter Black Holes: Perturbations and quasi-normal modes in the slow rotation limit
• Measuring the properties of nearly extremal black holes with gravitational waves
• AGILE Observations of the Gravitational-wave Source GW170817: Constraining Gamma-Ray Emission from a NS-NS Coalescence
• The massive Dirac equation in the Kerr-Newman-de Sitter and Kerr-Newman black hole spacetimes
• Polarization Modes of Gravitational Waves in Palatini Horndeski theory
• Non-trivial gravitational waves and structure formation phenomenology from dark energy
• Distinguishing Brans-Dicke-Kerr type naked singularities and black holes with their thin disk electromagnetic radiation properties
• Fortifying gravitational-wave tests of general relativity against astrophysical assumptions
• GRAPH mixing
• Classification of gravitational-wave glitches via dictionary learning
• The Gravitational Wave Stress-Energy (pseudo)-Tensor in Modified Gravity
• Complementary constraints on dark energy equation of state from strongly lensed gravitational wave
• Evidence for subdominant multipole moments and precession in merging black-hole-binaries from GWTC-2.1
• Are stellar--mass binary black hole mergers isotropically distributed?
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Minimal Theory of Bigravity: construction and cosmology
• Characterization of numerical relativity waveforms of eccentric binary black hole mergers
• Perturbative deflection angle for signal with finite distance and general velocities
• Vaidya and generalized Vaidya solutions by gravitational decoupling
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
• Implementing Tidal and Gravitational Wave Energy Losses in Few-body Codes: A Fast and Easy Drag Force Model
• Dark Matter Simulations with Primordial Black Holes in the Early Universe
• Quasinormal modes of black holes with a scalar hair in Einstein-Maxwell-dilaton theory
• Testing gravity of a disformal Kerr black hole in quadratic degenerate higher-order scalar-tensor theories by quasi-periodic oscillations
• Axial Quasi-Normal Modes of Scalarized Neutron Stars with Realistic Equations of State
• "Conserved charges" of the Bondi-Metzner-Sachs algebra in the Brans-Dicke theory
• Subaru Hyper Suprime-Cam Survey for An Optical Counterpart of GW170817
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Spin-orbit precession along eccentric orbits: improving the knowledge of self-force corrections and of their effective-one-body counterparts
• The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave Observatories
• Quasinormal mode frequencies and gravitational perturbations of spinning black holes in modified gravity through METRICS: The dynamical Chern-Simons gravity case
• Self-consistent effective-one-body theory for spinning binaries based on post-Minkowskian approximation
• Constraining spinning primordial black holes with global 21-cm signal
• Rapid and accurate parameter inference for coalescing, precessing compact binaries
• Improved Constraints on Modified Gravity with Eccentric Gravitational Waves
• Gravitational wave generation in a viable scenario of inflationary magnetogenesis
• Secular evolution of compact binaries revolving around a spinning massive black hole
• Gravitational Instability of Exotic Compact Objects
• Cogenesis of LIGO Primordial Black Holes and Dark Matter
• Quasi-normal modes of massless scalar fields for charged black holes in the Palatini-type gravity
• Probing black holes in a dark matter spike of M87 using quasinormal modes
• Observing the Shadows of Stellar-Mass Black Holes with Binary Companions
• Analogue simulation of gravitational waves in a 3+1 dimensional Bose-Einstein condensate
• Testing No-Hair Theorem by Quasi-Periodic Oscillations: the quadrupole of GRO J1655$-$40
• Perturbative deflection angle, gravitational lensing in the strong field limit and the black hole shadow
• The X-Ray Luminosity Function of Ultra Luminous X-Ray Sources in Collisional Ring Galaxies
• Gravitational self-force corrections to gyroscope precession along circular orbits in the Kerr spacetime
• A Search for Optical Emission from Binary-Black-Hole Merger GW170814 with the Dark Energy Camera
• Initial data for general relativistic simulations of multiple electrically charged black holes with linear and angular momenta
• Probing the Black Hole Merger History in Clusters using Stellar Tidal Disruptions
• Identifying correlations between LIGO's astronomical range and auxiliary sensors using lasso regression
• Gravitational wave constraints on planetary-mass primordial black holes using LIGO O3a data
• Gravitational waves from fast-spinning white dwarfs
• Polarization of gravitational waves in general teleparallel theories of gravity
• Electromagnetic Counterparts of Compact Binary Mergers
• Astrophysical Gravitational Waves in Conformal Gravity
• Decoherence of Gravitational Wave Oscillations in Bigravity
• Effect of gravitational wave on shadow of a Schwarzschild black hole
• Circularly polarized scalar induced gravitational waves from the Chern-Simons modified gravity
• Improvements in Gravitational-Wave Sky Localization with Expanded Networks of Interferometers
• Search for continuous gravitational waves from ten H.E.S.S. sources using a hidden Markov model
• Solving the relativistic inverse stellar problem through gravitational waves observation of binary neutron stars
• Radio Emission from Accreting Isolated Black Holes in Our Galaxy
• Effect of orbital eccentricity on the dynamics of precessing compact binaries
• Constraining Screened Modified Gravity by Space-borne Gravitational-wave Detectors
• Binary white dwarfs and decihertz gravitational wave observations: From the Hubble constant to supernova astrophysics
• Wave effect of gravitational waves intersected with a microlens field: a new algorithm and supplementary study
• Dirac perturbations on Schwarzschild-Anti-de Sitter spacetimes: Generic boundary conditions and new quasinormal modes
• Detection and characterization of spin-orbit resonances in the advanced gravitational wave detectors era
• Converting the signal-recycling cavity into an unstable optomechanical filter to enhance the detection bandwidth of gravitational-wave detectors
• $2+1$ Einstein-Klein-Gordon black holes by gravitational decoupling
• Horizon Surface Gravity in Corotating Black Hole Binaries
• Stochastic gravitational-wave background from spin loss of black holes
• From polarized gravitational waves to analytically solvable electromagnetic beams
• Primordial black holes in scalar field inflation coupled to the Gauss-Bonnet term with fractional power-law potentials
• Quasinormal modes of charged black holes in higher-dimensional Einstein-power-Maxwell theory
• Search for GeV Gamma-ray Counterparts of Gravitational Wave Events by CALET
• Particle Swarm Optimization based search for gravitational waves from compact binary coalescences: performance improvements
• A blind search for a common signal in gravitational wave detectors
• Constraining the Extra Polarization Modes of Gravitational Waves with Double White Dwarfs
• Model systematics in time domain tests of binary black hole evolution
• Primordial Black Holes from Affleck-Dine Mechanism
• Black Holes and Neutron Stars in Nearby Galaxies: Insights from NuSTAR
• The stepping-stone sampling algorithm for calculating the evidence of gravitational wave models
• Quasinormal Modes for Dynamical Black Holes
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• Template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and the first observation run of Advanced Virgo
• Evolution of dwarf galaxies hosting GW150914-like events
• Gravitational quasinormal modes of black holes in Einstein-aether theory
• Black Hole Mergers Induced by Tidal Encounters with a Galactic Centre Black Hole
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• Constraining the Neutron Star Radius with Joint Gravitational-Wave and Short Gamma-Ray Burst Observations of Neutron Star-Black Hole Coalescing Binaries
• Constraints on primordial black hole dark matter from Galactic center X-ray observations
• The impact of distant fly-bys on the rate of binary primordial black hole mergers
• Critical Emission from a High-Spin Black Hole
• Synergy between ground and space based gravitational wave detectors II: Localisation
• Black hole quasinormal modes in the era of LIGO
• Detecting Gravitational Self Lensing from Stellar-Mass Binaries Composed of Black Holes or Neutron Stars
• Spicing up the recipe for echoes from exotic compact objects: orbital differences and corrections in rotating backgrounds
• Long-Lived Quasinormal Modes and Quasi-Resonances around Non-Minimal Einstein-Yang-Mills Black Holes
• Analytical effective-one-body formalism for extreme-mass-ratio inspirals: eccentric orbits
• Energy Extraction via Magnetic Reconnection in Konoplya-Rezzolla-Zhidenko Parametrized Black Holes
• Gravitational waveforms and radiation powers of the triple system PSR J0337+1715 in modified theories of gravity
• Beyond the Hellings-Downs curve: Non-Einsteinian gravitational waves in pulsar timing array correlations
• Rainbow scattering of gravitational plane waves by a compact body
• Applying the effective-source approach to frequency-domain self-force calculations for eccentric orbits
• Exploring Critical Overdensity Thresholds in Inflationary Models of Primordial Black Holes Formation
• Motion deviation of test body induced by spin and cosmological constant in extreme mass ratio inspiral binary system
• High-energy neutrino emission subsequent to gravitational wave radiation from supermassive black hole mergers
• Generating Rotating Spacetime in Ricci-Based Gravity: Naked Singularity as a Black Hole Mimicker
• Common Envelope Evolution of Massive Stars
• Are fast radio bursts the most likely electromagnetic counterpart of neutron star mergers resulting in prompt collapse?
• Lecture notes on black hole binary astrophysics
• Black hole formation in relativistic Oscillaton collisions
• Niederer's transformation, time-dependent oscillators and polarized gravitational waves
• Matrix method for perturbed black hole metric with discontinuity
• Gravitational Wave Astronomy: Delivering on the Promises
• Structure formation with primordial black holes: collisional dynamics, binaries, and gravitational waves
• Condition for directly testing scalar modes of gravitational waves by four detectors
• High-order matrix method with delimited expansion domain
• Fluid pulsation modes and tidal deformability of anisotropic strange stars in light of the GW$170817$ event
• The future of gravitational theories in the era of the gravitational wave astronomy
• GW190521 formation scenarios via relativistic accretion
• Extraction of black hole coalescence waveforms from noisy data
• Binary black hole growth by gas accretion in stellar clusters
• Bondi mass with a cosmological constant
• Massive Graviton Geons
• Constraining the Gravitational-Wave Afterglow From a Binary Neutron Star Coalescence
• The best place and time to live in the Milky Way
• Spinning Particle Dynamics and ISCO in Covariant Loop Quantum Gravity
• Lensing magnification: gravitational waves from coalescing stellar-mass binary black holes
• Primordial black holes generated by fast-roll mechanism in non-canonical natural inflation
• Polarization Whorls from M87* at the Event Horizon Telescope
• Localization of Compact Binary Sources with Second Generation Gravitational-wave Interferometer Networks
• Searching for primordial black holes with stochastic gravitational-wave background in the space-based detector frequency band
• Polar Quasinormal Modes of Neutron Stars in Massive Scalar-Tensor Theories
• GW150914 peak frequency: a novel consistency test of strong-field General Relativity
• Finite-distance gravitational deflection of massive particles by a rotating black hole in loop quantum gravity
• GUP-corrected black holes: Thermodynamic properties, evaporation time and shadow constraint from EHT Observations of M87* and Sgr A*
• Time delay of timelike particles in gravitational lensing of Schwarzschild spacetime
• Parametrizations for tests of gravity
• Spin and Center of mass comparison between the PN approach and the asymptotic formulation
• Scalar induced gravitational waves from Chern-Simons gravity during inflation era
• Lensing rates of gravitational wave signals displaying beat patterns detectable by DECIGO and B-DECIGO
• Magnetic Braking and Damping of Differential Rotation in Massive Stars
• All-sky radiometer for narrowband gravitational waves using folded data
• Analytic computation of the secular effects of encounters on a binary: third-order perturbation, octupole, and post-Newtonian terms; steady-state distribution
• Rates of Short-GRB afterglows in association with Binary Neutron Star mergers
• Probing Screening and the Graviton Mass with Gravitational Waves
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Primordial Black Hole Formation in Non-Standard Post-Inflationary Epochs
• Dynamical signatures of black holes in massive Chern-Simons gravity: Quasibound modes and time evolution
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Geodesics, accretion disk, gravitational lensing, time delay, and effects on neutrinos induced by a non-commutative black hole
• Active platform stabilisation with a 6D seismometer
• Seismic Cross-coupling Noise in Torsion Pendulums
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• On-axis scattering of scalar fields by charged rotating black holes
• Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
• Gravitational waves without general relativity: A tutorial
• Antisymmetric tensor influence on charged black hole lensing phenomena and time delay
• Multi-messenger Gravitational Lensing
• Measuring deviations from the Kerr geometry with black hole ringdown
• Accelerated motion and the self-force in Schwarzschild spacetime
• Inspiral-Merger-Ringdown Consistency Tests with Higher Modes on Gravitational Signals from the Second Observing Run of LIGO and Virgo
• Extraction Energy From Charged Vaidya Black Hole Via Penrose Process
• Swift sky localization of gravitational waves using deep learning seeded importance sampling
• Scale-dependent slowly rotating black holes with flat horizon structure
• Dark Matter Signals on a Laser Interferometer
• H.E.S.S. follow-up observations of Binary Black Hole Coalescence events during the second and third Gravitational Waves observing runs of Advanced LIGO and Advanced Virgo
• Distribution of primordial black holes and 21cm signature
• Magnetic coupling to the Advanced Virgo payloads and its impact on the low frequency sensitivity
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• Enhancing the sensitivity of transient gravitational wave searches with Gaussian Mixture Models
• On the Inverse Spectrum Problem of Neutron Stars
• Constraint on the radius of five-dimensional dS spacetime with GW170817 and GRB 170817A
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
• Gravitational Self-Force Regularization in the Regge-Wheeler and Easy Gauges
• Non-commutativity in Hayward spacetime
• Evolution of the Black Hole Mass Function in Star Clusters from Multiple Mergers
• LISA Telescope: Phase noise due to pointing jitter
• A Challenge to Identify an Optical Counterpart of the Gravitational Wave Event GW151226 with Hyper Suprime-Cam
• Next-to-leading order spin-orbit effects in the equations of motion, energy loss and phase evolution of binaries of compact bodies in the effective field theory approach
• 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
• The H.E.S.S. Gravitational Wave Rapid Follow-up Program
• An Empirical Study of Contamination in Deep, Rapid, and Wide-Field Optical Follow-Up of Gravitational Wave Events
• Enhanced detection of high frequency gravitational waves using optically diluted optomechanical filters
• A six degree-of-freedom fused silica seismometer: Design and tests of a metal prototype
• On the gravitational lensing interpretation of three gravitational wave detections in the mass gap by LIGO and Virgo
• The evolution of a primordial binary black hole due to interaction with cold dark matter and the formation rate of gravitational wave events
• Identifying glitches near gravitational-wave signals from compact binary coalescences using the Q-transform
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
• Scalar induced gravitational waves in metric teleparallel gravity with the Nieh-Yan term
• Cosmological constraints from low-redshift data
• Quasinormal modes and echo effect of cylindrical anti-de Sitter black hole spacetime with a thin shell
• Polarization modes of gravitational waves in generalized Proca theory
• Measuring the primordial gravitational wave background in the presence of other stochastic signals
• Poisson-Arago spot for gravitational waves
• On spin optics for gravitational waves lensed by a rotating object
• Linearized modified gravity theories and gravitational waves physics in the GBD theory
• Fast Multipole Methods for $N$-body Simulations of Collisional Star Systems
• Observing the dark sector
• Exploring the CPT violation and birefringence of gravitational waves with ground- and space-based gravitational-wave interferometers
• Ground motion prediction at gravitational wave observatories using archival seismic data
• Gravitational Decoupling algorithm modifies the value of the conserved charges and thermodynamics properties in Lovelock Unique Vacuum theory
• String Memories ... Lost and Regained
• Gravitational Waves in the Presence of Viscosity
• Adaptive mesh refinement in binary black holes simulations
• Searching for high-frequency gravitational waves by ground high field magnetic resonant sweepings
• Characterization of low-significance gravitational-wave compact binary sources
• Time evolution of the local gravitational parameters and gravitational wave polarizations in a relativistic MOND theory
• Very extreme mass-ratio bursts in the Galaxy and neighbouring galaxies in relation to space-borne detectors
• Detection possibility of continuous gravitational waves from rotating magnetized neutron stars
• Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term
• Scalar Charges and Scaling Relations in Massless Scalar-Tensor Theories
• Incorporating information from LIGO data quality streams into the PyCBC search for gravitational waves
• Comments on Gravitoelectromagnetism of Ummarino and Gallerati in "Superconductor in a weak static gravitational field" vs Other Versions
• New gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole: gyroscope precession
• Supporting High-Performance and High-Throughput Computing for Experimental Science
• Inverse spectrum problem for quasi-stationary states
• Mechanisms for producing Primordial Black Holes from Inflationary Models Beyond Fine-Tuning
• Weighing the IMBH candidate CO-0.40-0.22* in the Galactic Centre
• A Complete Analytic Gravitational Wave Model for Undergraduates
• Constraining the history of reheating with the NANOGrav 15-year data
• Bayesian inference for binary neutron star inspirals using a Hamiltonian Monte Carlo Algorithm
• Python Open Source Waveform Extractor (POWER): An open source, Python package to monitor and post-process numerical relativity simulations
• Gravitational waves from strong first order phase transitions
• Sensitivity of third-generation interferometers to extra polarizations in the Stochastic Gravitational Wave Background
• Inspirals into a charged black hole
• Solitons and black hole in shift symmetric scalar-tensor gravity with cosmological constant
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• A feasibility study on the photometric detection of quiescent black hole X-ray binaries
• Quantum Field Theory with Classical Sources - Linearized Quantum Gravity
• Strongly Magnetized Hot QCD Matter and Stochastic Gravitational Wave Background
• The Evolution of Kicked Stellar-Mass Black Holes in Star Cluster Environments
• Constraining the non-Einsteinian polarizations of gravitational waves by pulsar timing array
• Reconstruction of the neutron star equation of state from $w$-quasinormal modes spectra with a piecewise polytropic meshing and refinement method
• An Alternative Channel For High-Mass Binary Black Holes-----Dark Matter Accretion Onto Black Hole
• Exclusion of standard $\hslash \omega$ gravitons by LIGO observation
• Gravitational Waves as a Probe of the Extra Dimension
• Effect of inhomogeneities on the propagation of gravitational waves from binaries of compact objects
• Astrophysical signal consistency test adapted for gravitational-wave transient searches
• Towards a robust and reliable deep learning approach for detection of compact binary mergers in gravitational wave data
• An independent search of gravitational waves in the first observation run of advanced LIGO using cross-correlation
• Long term measurements from the Mátra Gravitational and Geophysical Laboratory
• Polarization modes of gravitational waves in general modified gravity: General metric theory and general scalar-tensor theory
• Improving performance of SEOBNRv3 by $\sim$300x
• Gravitational waves from SGRs and AXPs as fast-spinning white dwarfs
• Short Gamma-Ray Bursts and Gravitational-Wave Observations from Eccentric Compact Binaries
• Einstein-Cartan-Dirac gravity with $U(1)$ symmetry breaking
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds
• Bouncing behavior in $f(R,L_m)$ gravity: Phantom crossing and energy conditions
• Testing the anisotropy of the universe using the simulated gravitational wave events from advanced LIGO and Virgo
• Gravitational Waves and Degrees of Freedom in Higher Derivative Gravity
• Deflection angle with electromagnetic interaction and gravitational-electromagnetic dual lensing
• Constructive summation of the (2,2) quasi normal mode from a population of black holes
• Constraints on Scalar-Tensor Theory of Gravity by Solar System Tests
• Posterior samples of the parameters of binary black holes from Advanced LIGO, Virgo's second observing run
• Analytical analysis on the orbits of Taiji spacecrafts
• Conformal gravity: light deflection revisited and the galactic rotation curve failure
• A phase-sensitive optomechanical amplifier for quantum noise reduction in laser interferometers
• Echoes of axial gravitational perturbations in stars of uniform density
• Gravitational wave modes in matter
• Imprint of Early Dark Energy in Stochastic Gravitational Wave Background
• A Coincidence Null Test for Poisson-Distributed Events
• Supernova and prompt gravitational-wave precursors to LIGO gravitational-wave sources and short-GRBs
• The Effective Fluid approach for Modified Gravity and its applications
• Hierarchical search strategy for the efficient detection of gravitational waves from non-precessing coalescing compact binaries with aligned-spins
• Quadrupolar power radiation by a binary system in de Sitter Background
• Electromagnetic emissions from near-horizon region of an extreme Kerr-Taub-Nut black hole
• Fab Four Effective Field Theory Treatment
• Compact objects in quadratic Palatini gravity generated by a free scalar field
• Gravitational waves in conformal gravity
• Radio Transients from Newborn Black Holes
• Fundamental Relations between Measurement, Radiation and Decoherence in Gravitational Wave Laser Interferometer Detectors
• Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background
• Tailoring cosmologies in cubic shift-symmetric Horndeski gravity
• GW170817: A Neutron Star Merger in a Mass-Transferring Triple System
• Application of a Zero-latency Whitening Filter to Compact Binary Coalescence Gravitational-wave Searches
• Black Hole Spin Axis in Numerical Relativity
• An Effective Model for the Quantum Schwarzschild Black Hole: Weak Deflection Angle, Quasinormal Modes and Bounding of Greybody Factor
• Gravitational waves in Modified Gauss-Bonnet Gravity
• - Gravitational Waves - A Review on the Conceptual Foundations of Gravitational Radiation
• The growth of stellar mass black hole binaries trapped in an accretion disk of active galactic nuclei
• Source localizations with the network of space-based gravitational wave detectors
• Nonorthogonal wavelet transformation for reconstructing gravitational wave signals
• Classifying Lensed Gravitational Waves in the Geometrical Optics Limit with Machine Learning
• Impact of overlapping signals on parameterized post-Newtonian coefficients in tests of gravity
• Ringdown Spectroscopy of Rotating Black Holes Pierced by Cosmic Strings
• Gravitational-Wave Geodesy: A New Tool for Validating Detection of the Stochastic Gravitational-Wave Background
• A New Possible Accretion Scenario for Ultra-Luminous X-ray Sources
• Schwarzschild Fuzzball and Explicitly Unitary Hawking Radiations
• GW170817 event rules out general relativity in favor of vector gravity
• Can we detect quantum gravity with compact binary inspirals?
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• Numerically modeling Brownian thermal noise in amorphous and crystalline thin coatings
• Astrophysical insights into magnetic Penrose process around parameterized Konoplya-Rezzolla-Zhidenko black hole
• A new look at the Bondi-Sachs energy-momentum
• Novel Hairy Black Hole Solutions in Einstein-Maxwell-Gauss-Bonnet-Scalar Theory
• Gravitational Waves From No-Scale Supergravity
• Charged scalar-tensor solitons and black holes with (approximate) Anti-de Sitter asymptotics
• Motion of test particle in rotating boson star
• Parametrized black holes: Scattering investigation
• A Note on QR-Based Model Reduction: Algorithm, Software, and Gravitational Wave Applications
• Quantum coherence of relic gravitons and Hanbury Brown-Twiss interferometry
• Hair-dressing Horndeski: an approach to hairy solutions in cubic Horndeski gravity
• Model-independent discovery prospects for primordial black holes at LIGO
• Estimation of the gravitational wave polarizations from a non template search
• Reconstruction method in the kinetic gravity braiding theory with shift-symmetric
• Bayesian Inference Analysis of Unmodelled Gravitational-Wave Transients
• Detection of gravitational wave mixed polarization with single space-based detectors
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Cosmological bounces, cyclic universes, and effective cosmological constant in Einstein-Cartan-Dirac-Maxwell theory
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Black hole spectroscopy for KAGRA future prospect in O5
• Scalar-tensor black holes in an expanding universe
• Quasinormal modes of scalar field coupled to Einstein's tensor in the non-commutative geometry inspired black hole
• Effect of electric interaction on the deflection and gravitational lensing in the strong field limit
• Fundamental Physics and Cosmology with TianQin
• Scalar polarization window in gravitational-wave signals
• A new representation of vacuum Lovelock solutions in $d=2N+1$ dimensions: Black holes with an integrable singularity and regular black holes
• Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
• Binary-binary scattering in the secular limit
• Gravitational self-force corrections to tidal invariants for particles on eccentric orbits in a Schwarzschild spacetime
• Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
• Polarization modes of gravitational waves in general Einstein-vector theory
• Dilatonic Imprints on Exact Gravitational Wave Signatures
• Gravitational self-force corrections to tidal invariants for spinning particles on circular orbits in a Schwarzschild spacetime
• J1342+0928 Supports the Timeline in the R_h=ct Cosmology
• Phenomenological Inclusion of Alternative Dispersion Relations to the Teukolsky Equation and its Application to Bounding the Graviton Mass with Gravitational-wave Measurements
• Electromagnetic counterparts to gravitational wave events from Gaia
• Applications of the close-limit approximation: horizonless compact objects and scalar fields
• Towards a Polarisation Prediction for LISA via Intensity Interferometry
• Selected spherical photon orbits around a deformed Kerr black hole
• Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
• Gravitational Wave Signal Extraction Against Non-Stationary Instrumental Noises with Deep Neural Network
• Characteristics of interaction between Gravitons and Photons
• Gravitational radiation by magnetic field: application to millisecond magnetars
• Measuring the Black Hole Mass Spectrum from Redshifts of aLIGO Binary Merger Events
• Gravitational waves in massive conformal gravity
• A Case Study of On-the-Fly Wide-Field Radio Imaging Applied to the Gravitational-wave Event GW 151226
• Scalar induced gravitational waves in chiral scalar-tensor theory of gravity
• Light propagation in the field of the N-body system and the application in the TianQin mission
• Waveforms from Amplitudes
• Spline Based Search Method For Unmodeled Transient Gravitational Wave Chirps
• Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes
• Gravitational Radiation from Close Binaries with Time-Varying Masses
• Strong gravitational lensing of rotating regular black holes in non-minimally coupled Einstein-Yang-Mills theory
• Analytical and numerical treatment of perturbed black holes in horizon-penetrating coordinates
• Inverse problem of analog gravity systems
• Revisiting scalar and tensor perturbations in a nonlocal gravity
• On the Expected Production of Gravitational Waves During Preheating
• Follow-up procedure for gravitational wave searches from isolated neutron stars using the time-domain $\mathcal{F}$-statistic method
• Formation rate of LB-1-like systems through dynamical interactions
• Strong and weak lensing of Gravitational Waves: a semi-analytical approach
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• Spiky CMB distortions from primordial bubbles
• Reissner-Nordström perturbation framework with gravitational wave applications
• Enhancing gravitational waveform models through dynamic calibration
• On the possible electromagnetic manifestations of merging black holes
• Unveiling the Universe with Emerging Cosmological Probes
• An unknown branch of the total-transmission modes for the Kerr-geometry
• Viscous attenuation of gravitational waves propagating through an inhomogeneous background
• Gravitational wave polarization from combined Earth-space detectors
• Untargeted Bayesian search of anisotropic gravitational-wave backgrounds through the analytical marginalization of the posterior
• Singularities of plane gravitational waves and their memory effects
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Gravitational self-force corrections to tidal invariants for particles on circular orbits in a Kerr spacetime
• CAMELOT - Concept study and early results for onboard data processing and GPS-based timestamping
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• Massive scalar field perturbations of 4D de Sitter Einstein-Gauss-Bonnet black holes
• Einstein-Horndeski gravity and the ultra slowly evaporating black hole
• Reducing the number of templates for aligned-spin compact binary coalescence gravitational wave searches using metric-agnostic template nudging
• Search for the optical counterpart of the GW170814 gravitationalwave event with the VLT Survey Telescope
• Axisymmetric Hydrodynamics in Numerical Relativity Using a Multipatch Method
• Identifying extra high frequency gravitational waves generated from oscillons with cuspy potentials using deep neural networks
• Boosted Kerr black holes in general relativity
• Strong Equivalence Principle and Gravitational Wave Polarizations in Horndeski Theory
• Probing charge of compact objects with gravitational microlensing of gravitational waves
• Galerkin-Collocation domain decomposition method for arbitrary binary black holes
• Average nonlinear dynamics of particles in gravitational pulses: effective Hamiltonian, secular acceleration, and gravitational susceptibility
• Likelihood for a Network of Gravitational-Wave Detectors with Correlated Noise
• On the Gravitational Wave to Matter Coupling of Superfluid Fermi Gases Near Unitarity
• Medium-band observation of the neutrino emitting blazar, TXS 0506+056
• Optimizing the Placement of Numerical Relativity Simulations using a Mismatch Predicting Neural Network
• Measurement of Tidal Deformability in the Gravitational Wave Parameter Estimation for Nonspinning Binary Neutron Star Mergers
• New total transmission modes of the Kerr geometry with Schwarzschild limit frequencies at complex infinity
• Angular instability in high optical power suspended cavities
• Merger of multiple accreting black holes concordant with gravitational wave events
• Sunyaev-Zel'dovich anisotropy due to Primordial black holes
• Perturbative deflection angles of timelike rays
• Gravitational Waves from Mirror World
• Testing black holes in a perfect fluid dark matter environment using quasinormal modes
• Schumann resonance transients and the search for gravitational waves
• Time delay in the strong field limit for null and timelike signals and its simple interpretation
• Scalar Stochastic Gravitational-Wave Background in Brans-Dicke Theory of Gravity
• Quantum Effects in Galileon Black Holes
• Minimally modified gravity with auxiliary constraints formalism
• Strong-field gravitational lensing by black holes
• Gravitational waves from inspiralling compact binaries in conformal gravity
• Quansinormal modes of static and spherically symmetric black holes with the derivative coupling
• Energy flux and waveforms by coalescing spinless binary system in effective one-body theory
• Black holes in General Relativity and beyond
• Quantum noise cancellation in asymmetric speed meters with balanced homodyne readout
• Gravitational Wave Propagation and Polarizations in the Teleparallel analog of Horndeski Gravity
• Quasinormal Modes by Improved Matrix Method and Weighted Residual Method
• Observational constraint on axion dark matter with gravitational waves
• Constraining Black Hole Populations in Globular Clusters using Microlensing: Application to Omega Centauri
• Mass octupole and current quadrupole corrections to gravitational wave emission from close hyperbolic encounters
• Phase transition and stiffer core fluid in neutron stars: Effects on stellar configurations, dynamical stability, and tidal deformability
• GRB 180128A: A Second Magnetar Giant Flare Candidate from the Sculptor Galaxy
• Extragalactic Magnetar Giant Flare GRB 231115A: Insights from Fermi/GBM Observations
• Escape, bound and capture geodesics in local static coordinates in Schwarzschild spacetime
• Multipolar Particles in Helically Symmetric Spacetimes
• Testing dispersion of gravitational waves from eccentric extreme-mass-ratio inspirals
• Gravitational wave scattering theory without large-distance asymptotics
• Primordial black holes in SB SUSY Gauss-Bonnet inflation
• Imprints of Early Universe on Gravitational Waves from First-Order Phase Transition in QCD
• lenscat: a Public and Community-Contributed Catalog of Known Strong Gravitational Lenses
• Effect of induced seismicity on advanced gravitational wave interferometers
• Corrections to the gravitational wave phasing
• Multipole analysis on gyroscopic precession in $f(R)$ gravity with irreducible Cartesian tensors
• CLAP for modified gravity: scalar instabilities in binary black hole spacetimes
• Rio: A new computational framework for accurate initial data of binary black holes
• Gravitational Wave luminosity distance in viscous cosmological models
• The 1.5 post-Newtonian radiative quadrupole moment in the context of a nonlocal field theory of gravity
• Afterglows and Macronovae Associated with Nearby Low-Luminosity Short-Duration Gamma-Ray Bursts
• Probing the formation of the seeds of supermassive black holes with gravitational waves
• Driving unmodelled gravitational-wave transient searches using astrophysical information
• Inferring black-hole orbital dynamics from numerical-relativity gravitational waveforms
• Gravitational wave detector OGRAN as multi-messenger project of RAS-MSU
• Very high frequency gravitational waves from magnetars and gamma-ray burst
• Traversable wormholes with multiple unstable critical curves
• Exact ghost-free bigravitational waves
• Probing nontensorial gravitational waves with a next-generation ground-based detector network
• A Possible Quantum Gravity Hint in Binary Black Hole Merger
• Recent LIGO-Virgo discoveries
• Gravitational Wave Signatures of Primordial Black Hole Reheating in Upcoming Interferometry Missions
• Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
• Microlensing of dark matter models in the Milky Way
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• Gravitational Wave Searches with Pulsar Timing Arrays. I: Cancellation of Clock and Ephemeris Noises
• Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
• Unveiling the existence of nontensorial gravitational-wave polarizations from individual supermassive black hole binaries with pulsar timing arrays
• Trumpet Initial Data for Boosted Black Holes
• Multipole analysis for linearized $f(R)$ gravity with irreducible Cartesian tensors
• Multipole analysis for linearized $f(R,\mathcal{G})$ gravity with irreducible Cartesian tensors
• Arm locking in conjunction with time-delay interferometry
• Random projections in gravitational wave searches of compact binaries
• Can a "pure vector" gravitational wave mimic a "pure tensor" one?
• Intermediate Mass Black Holes: A brief review
• Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity
• Angular Momentum Loss for a Binary System in Einstein-Æther Theory
• Phase decomposition of the template metric for continuous gravitational-wave searches
• The gravitational Higgs mechanism and resulting smoking gun effects
• A novel multi-layer modular approach for real-time fuzzy-identification of gravitational-wave signals
• Maxwell Fields in Boosted Kerr Black Holes
• A protocol of potential advantage in the low frequency range to gravitational wave detection with space based optical atomic clocks
• Earth rotation and time-domain reconstruction of polarization states for continuous gravitational waves from a known pulsar
• Energy emission from high curvature region and its backreation
• Lanczos equation on light-like hypersurfaces in a cosmologically viable class of kinetic gravity braiding theories
• On the waveform of the scalar induced gravitational waves
• A General Overview for Localizing Short Gamma-ray Bursts with a CubeSat Mega-Constellation
• Interferometer Euro-Asian Network: Detection Characteristics for Signals of Known Shape
• On the Signal Processing Operations in LIGO signals
• Limits on the Electro-Magnetic Counterpart of Binary Black Hole Coalescence at Visible Wavelengths
• Pattern of lensed chirp gravitational wave signal and its implication on the mass and position of lens
• Design and experimental demonstration of a laser modulation system for future gravitational-wave detectors
• Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
• Modified gravity with disappearing cosmological constant
• Exotic compact object behavior in black hole analogues
• No hair theorem for bound-state massless static scalar fields outside horizonless Neumann compact stars
• Stochastic gravitational wave background from accreting primordial black hole binaries during early inspiral stage
• $M/R$ estimates for two neutron stars in LMXBs with possible r-mode frequencies detected
• First joint observation by the underground gravitational-wave detector, KAGRA, with GEO600
• Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Thermodynamic topology of dyonic AdS black holes with quasitopological electromagnetism in Einstein-Gauss-Bonnet gravity
• An estimate of the gravitational-wave background from the observed cosmological distribution of quasars
• Gravitational Wave Emission from Close-in Strange Quark Planets Around Strange Stars with Magnetic Interactions
• Testing Lorentz symmetry with space-based gravitational-wave detectors
• Estimating the Final Spin of Binary Black Holes Merger in STU Supergravity
• Status of the Advanced Virgo gravitational-wave detector
• An Interactive Gravitational-Wave Detector Model for Museums and Fairs
• Holographic Bound on Area of Compact Binary Merger Remnant
• Deflection of charged massive particles by a four-dimensional charged Einstein-Gauss-Bonnet black hole
• Gravitational waves in gauge theory gravity with a negative cosmological constant
• GW170814: Gravitational wave polarization analysis
• Orbital Stability Study of the Taiji Space Gravitational Wave Detector
• Long Journey toward the Detection of Gravitational Waves and New Era of Gravitational Wave Astrophysics
• Prospects for estimating parameters from gravitational waves of superspinar binaries
• Unveiling the enigma of ATLAS17aeu
• Multipole analysis in the radiation field for linearized $f(R)$ gravity with irreducible Cartesian tensors
• Particle Dynamics on Test Papapetrou Fields of Vacuum Spacetimes
• Cosmoparticle physics of dark matter
• Primary gravitational waves at high frequencies I: Origin of suppression in the power spectrum
• Surprises from the spins: astrophysics and relativity with detections of spinning black-hole mergers
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Bounds from multi-messenger astronomy on the Super Heavy Dark Matter
• Coalescence of Kerr Black Holes: Binary Systems from GW150914 to GW170814
• Thermal noise of beam splitters in laser gravitational wave detectors
• Testing the variation of the fine structure constant with strongly lensed gravitational waves
• Looking for ancillary signals around GW150914
• Quantum gravity phenomenology from the perspective of quantum general relativity and quadratic gravity
• Reanalysis of LIGO black-hole coalescences with alternative prior assumptions
• Numerical Approach for Corvino-Type Gluing of Brill-Lindquist Initial Data
• Light-like shockwaves in scalar-tensor theories
• Dark matter influence on black hole objects thermodynamics
• Long-Range Quantum Gravity
• Higher order mimetic gravity after GW170817
• Magnetohydrodynamic waves excited by a coupling between gravitational waves and a strongly magnetized plasma in binaries of neutron stars
• Gravitational-wave signatures of nonviolent nonlocality
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• A new experiment for the gravitational waves detection
• Gauge-invariant gravitational waves in matter beyond linearized gravity
• Laser Interferometer in Presence of Scalar field on Gravitational Wave Background
• Multi-detector null-stream-based ${\chi }^2$ statistic for compact binary coalescence searches
• Gravitational slingshots around black holes in a binary
• Supernovae in massive binaries and compact object mergers near supermassive black holes
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Tidal forces around the Letelier-Alencar cloud of strings black hole
• Rotations of the polarization of a gravitational wave propagating in Universe
• Astrophysical uncertainties challenge 21-cm forecasts: A primordial black hole case study
• Echoes and quasinormal modes of asymmetric black bounces
• Small Spins of Primordial Black Holes from Random Geometries: Bekenstein-Hawking Entropy and Gravitational Wave Observations
• Spin dynamics of moving bodies in rotating black hole spacetimes
• Probing the post-Minkowskian approximation using recursive addition of self-interactions
• Convenient filtering techniques for LIGO strain of the GW150914 event
• Universal time delay in static spherically symmetric spacetimes for null and timelike signals
• Scalar-induced gravitational waves in spatially covariant gravity
• Piecewise polytropic meshing and refinement method for the reconstruction of the neutron star equation of state using tidal deformabilities and constraints in the piecewise polytropic parameters given by the GW170817 event
• Analytical analysis on the orbits of Taiji spacecrafts to infinite order of the orbital eccentricity
• Gravitational dynamics in a 2+1+1 decomposed spacetime along nonorthogonal double foliations: Hamiltonian evolution and gauge fixing
• Strong gravitational lensing of a five-dimensional charged, equally rotating black hole with a cosmological constant
• Gravitational wave pulse and memory effects for hairy Kiselev black hole and its analogy with Bondi-Sachs formalism
• Independent Component Analysis for Signal Crosstalk Elimination in Infrared Interferometry
• Tachyonic Instability of Reissner-Nordström-Melvin Black Holes in Einstein-Maxwell-Scalar Theory
• Revisiting Flat Rotation Curves in Chern-Simons Modified Gravity
• On the stability of covariant BSSN formulation
• Hairy black holes in extended Einstein-Maxwell-scalar theories with magnetic charge and kinetic couplings
• Imprints of the redshift evolution of double neutron star merger rate on the signal to noise ratio distribution
• Constructing Regular Lovelock Black Holes with degenerate vacuum and $\Lambda <0$, using the gravitational tension. Shadow analysis
• Physical modelling of galaxy clusters and Bayesian inference in astrophysics
• Constraining black-hole horizon effects by LIGO-Virgo detections of inspiralling binary black holes
• Gravitomagnetism and Gravitational Waves in Galileo-Newtonian Physics
• Axion Dark Matter Archaeology with Primordial Gravitational Waves
• A no-go theorem for regular black holes
• Probing the conformal invariance around the nonsingular static spherical black holes with waves
• Cosmological coupled black holes immersed in dark sector
• The Response of Optical Fibres to Gravitational Waves
• Challenging theories of gravitation: dark matter, compact objects and gravitational waves
• Gravitational waves in massive Horndeski theory with a potential
• Optimizing signal recycling for detecting a stochastic gravitational-wave background
• Particle Creation in a Linear Gravitational Wave Background
• Lensing by primordial black holes: constraints from gravitational wave observations
• Two body dynamics in a quadratic modification of general relativity
• Phenomenologically viable gravitational theory based on a preferred foliation without extra modes
• Perturbations of Einstein--Maxwell--phantom spacetime: Instabilities of charged Ellis--Bronnikov wormholes and quasinormal modes of black holes
• Population III Star Formation in an X-ray background: I. Critical Halo Mass of Formation and Total Mass in Stars
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Laser interferometry based on atomic coherence
• A quantisation procedure in the presence of an initial Kasner singularity: primordial gravitational waves from triaxially anisotropic pre-inflation
• Genetic-algorithm-optimized neural networks for gravitational wave classification
• Constructing balanced equations of motion for particles in general relativistic theories: the general case
• Ringing Black Hole is Superradiant: Ultra-light Scalar Field
• Spin precession of binary neutron stars with magnetic dipole moments
• The CUBES Science Case
• Cosmic expansion history analysis with Hubble parametrization in $Q^n$ gravity
• Tidal deformations of compact objects and gravitational wave emission
• Performance comparison of multi-detector detection statistics in targeted compact binary coalescence GW search
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Effect of nonlinear electrodynamics on polarization distribution around black hole
• Statistical biases in parametrized searches for gravitational-wave polarizations
• Calibrating systematic errors in the distance determination with the luminosity-distance space large scale structure of dark sirens and its potential applications
• Complementary signatures of $\alpha -$attractor inflation in CMB and cosmic string Gravitational Waves
• A New Set of Maxwell-Lorentz Equations and Rediscovery of Heaviside-Maxwellian (Vector) Gravity from Quantum Field Theory
• Particle Physics with Gravitational Wave Detector Technology
• Constraints on generalized Eddington-inspired Born-Infeld branes
• About the Power Spectrum Of Primordial Gravitational Waves
• Constructing balanced equations of motion for particles in general relativity: the harmonic gauge case
• Back reaction of the gravitational radiation on the metric of spacetime
• Sky localization and polarization mode reconstruction of gravitational waves from GW170104 and GW150914
• Tests of scalar polarizations with multi-messenger events
• On the ease of excitation of black hole ringing: Quantifying the importance of overtones by the excitation factors
• Superradiant scattering of massive scalar field due to magnetically charged rotating black hole
• Investigation of infrasound noise background at Mátra Gravitational and Geophysical Laboratory (MGGL)
• Gravitational wave signature of a mini creation event (MCE)
• Wave Front Sensing demodulated at the difference frequency between two phase-modulation sidebands in a compound interferometer configuration for a gravitational-wave detector
• One-Dimensional Primordial Gravitational Waves In Pure Quadratic Gravity
• Quantum Physics in Space
• Black hole solutions with a linear equation of state in Hořava gravity and Einstein--æther theory
• Quasinormal Modes of Near-Extremal Black Holes and Black Strings in Massive Gravity Background
• Evaluation of microseismic motion at the KAGRA site based on ocean wave data
• Detecting the processes of colliding plane gravitational waves by electromagnetic response signals
• Parameterized tests of general relativity with gravitational wave generation and propagation
• Gravity Induced Quantum Interference on Gravitational Wave Background
• Generating Event Triggers Based on Hilbert-Huang Transform and Its Application to Gravitational-Wave Data
• Do photons travel faster than gravitons?
• Primordial black holes and uncertainties in the choice of the window function
• P-stars in the gravitational wave era
• Gravitational wave seismology of charged strange stars in the Cowling approximation: the fluid pulsation modes
• Multi-Messenger Observations of GRBs: The GW connection
• The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
• Aspects of astrophysical particle production and beyond the Standard Model phenomenology
• 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
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Analytical solutions of bound timelike geodesic orbits in effective-one-body frame
• Terrestrial Laser Interferometers
• A new measure for the comparison of signals without templates and the detection of gravitational polarization in the GW150914 event
• Gravitational waves in Cubic Metric-Affine Gravity
• Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
• New Insights into the Nature of Nonlinear Gravitational Waves
• From Rare Events to a Population: Discovering Overlooked Extragalactic Magnetar Giant Flare Candidates in Archival Fermi Gamma-ray Burst Monitor Data
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• A Carillon of Black Holes
• Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves
• Existence of conserved quantities and their algebra in curved spacetime
• A Novel Search Technique for Low-Frequency Periodic Gravitational Waves
• Quantum Enhanced Interferometer for Kilohertz Gravitational Wave Detection
• Primordial gravitational waves: Model effects on time evolution and spectrum
• A viable relativistic scalar theory of gravitation
• Interaction between gravitational waves and trapped Bose-Einstein condensates
• Search For Electron-Antineutrinos Associated With Gravitational-Wave Events GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817 at Daya Bay
• Null-stream-based Bayesian Unmodeled Framework to Probe Generic Gravitational-wave Polarizations
• A template-free approach for waveform extraction of gravitational wave events
• A Gravitational Wave Background from Primordial Black Hole Lattices in Matter Dominated Era
• Topological dressing method for the Einstein-Maxwell equations
• Inverse compton scattered merger-nova: late X-ray counterpart of gravitational wave signals from NS-NS/BH mergers
• Analyses of residual accelerations for TianQin based on the global MHD simulation
• Cosmology of the interacting Cubic Galileon
• Gravitational Wave Detection and Information Extraction via Neural Networks
• An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
• Gravitational waves from generalized newtonian sources
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Linear perturbations of dyonic black holes in the lowest-order $U(1)$ gauge-invariant scalar-vector-tensor theories