Physics, Astrophysics and Cosmology with Gravitational Waves

Abstract

Gravitational wave detectors are already operating at interesting sensitivity levels, and they have an upgrade path that should result in secure detections by 2014. We review the physics of gravitational waves, how they interact with detectors (bars and interferometers), and how these detectors operate. We study the most likely sources of gravitational waves and review the data analysis methods that are used to extract their signals from detector noise. Then we consider the consequences of gravitational wave detections and observations for physics, astrophysics, and cosmology.

137 pages, 16 figures, Published version <http://www.livingreviews.org/lrr-2009-2>

References in corpus (81)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
• Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
• Primordial Nucleosynthesis in the Precision Cosmology Era
• Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA
• Large Merger Recoils and Spin Flips From Generic Black-Hole Binaries
• Total recoil: the maximum kick from nonspinning black-hole binary inspiral
• Observation of squeezed light with 10dB quantum noise reduction
• Inspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis
• A massive binary black-hole system in OJ287 and a test of general relativity
• Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole
• Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects
• Phenomenological template family for black-hole coalescence waveforms
• Coherent method for detection of gravitational wave bursts
• Toward faithful templates for non-spinning binary black holes using the effective-one-body approach
• Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes
• Magnetar-like Emission from the Young Pulsar in Kes 75
• Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries
• Gemini and Hubble Space Telescope Evidence for an Intermediate Mass Black Hole in omega Centauri
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• On the final spin from the coalescence of two black holes
• Recoil velocities from equal-mass binary black-hole mergers: a systematic investigation of spin-orbit aligned configurations
• Getting a kick out of numerical relativity
• Estimating the final spin of a binary black hole coalescence
• Gravitational Wave Detection by Interferometry (Ground and Space)
• LISA detections of massive black hole inspirals: parameter extraction errors due to inaccurate template waveforms
• Exploring black hole superkicks
• Upper limits on gravitational wave emission from 78 radio pulsars
• Gravitational Waves from Warped Spacetime
• Implications for the Origin of GRB 070201 from LIGO Observations
• High-spin binary black hole mergers
• Comparing Effective-One-Body gravitational waveforms to accurate numerical data
• A data-analysis driven comparison of analytic and numerical coalescing binary waveforms: nonspinning case
• Accurate Effective-One-Body waveforms of inspiralling and coalescing black-hole binaries
• Probing the non-linear structure of general relativity with black hole binaries
• Faithful Effective-One-Body waveforms of equal-mass coalescing black-hole binaries
• Tests of Bayesian Model Selection Techniques for Gravitational Wave Astronomy
• The final spin from the coalescence of aligned-spin black-hole binaries
• Generic Gravitational Wave Signals from the Collapse of Rotating Stellar Cores
• The Einstein@Home search for periodic gravitational waves in LIGO S4 data
• Merger of black hole-neutron star binaries in full general relativity
• A New Mechanism for Gravitational Wave Emission in Core-Collapse Supernovae
• Coherent network analysis technique for discriminating gravitational-wave bursts from instrumental noise
• The LISA verification binaries
• Search for a stochastic background of 100-MHz gravitational waves with laser interferometers
• Gravitational waves from inspiralling compact binaries: hexagonal template placement and its efficiency in detecting physical signals
• Binary black hole spectroscopy
• Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
• Relativistic Binary Pulsar B1913+16: Thirty Years of Observations and Analysis
• Localizing coalescing massive black hole binaries with gravitational waves
• LISA observations of supermassive black holes: parameter estimation using full post-Newtonian inspiral waveforms
• Final spin of a coalescing black-hole binary: an Effective-One-Body approach
• Intermediate-mass black holes in colliding clusters: Implications for lower-frequency gravitational-wave astronomy
• Measurement of Quantum Fluctuations in Geometry
• A Bayesian approach to the follow-up of candidate gravitational wave signals
• Coherent Bayesian inference on compact binary inspirals using a network of interferometric gravitational wave detectors
• Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals
• Blandford's Argument: The Strongest Continuous Gravitational Wave Signal
• MCMC Exploration of Supermassive Black Hole Binary Inspirals
• Results of the IGEC-2 search for gravitational wave bursts during 2005
• A geometric algorithm for efficient coincident detection of gravitational waves
• Sensitivity of the spherical gravitational wave detector MiniGRAIL operating at 5 K
• Assigning confidence to inspiral gravitational wave candidates with Bayesian model selection
• Higher harmonics increase LISA's mass reach for supermassive black holes
• Catching Super Massive Black Hole Binaries Without a Net
• Testing the Accuracy and Stability of Spectral Methods in Numerical Relativity
• Extracting galactic binary signals from the first round of Mock LISA Data Challenges
• Robust Bayesian detection of unmodelled bursts
• The Polarization of the Cosmic Microwave Background Due to Primordial Gravitational Waves
• Parameter estimation of coalescing supermassive black hole binaries with LISA
• Detecting extreme mass ratio inspiral events in LISA data using the Hierarchical Algorithm for Clusters and Ridges (HACR)
• High frequency oscillations during magnetar flares
• Searching for Massive Black Hole Binaries in the first Mock LISA Data Challenge
• Improved Hough search for gravitational wave pulsars
• Principles of wide bandwidth acoustic detectors and the single-mass DUAL detector
• Current status of Japanese detectors
• Detecting gravitational waves from inspiraling binaries with a network of detectors : coherent versus coincident strategies
• Automatic Bayesian inference for LISA data analysis strategies
• Detecting gravitational waves from inspiraling binaries with a network of detectors : coherent strategies by correlated detectors
• Gravitational Waves from Core-Collapse Supernovae
• Gravitational waves from coalescing massive black holes in young dense clusters

Cited by in corpus (582)

• The Confrontation between General Relativity and Experiment
• A Massive Pulsar in a Compact Relativistic Binary
• Quasinormal modes of black holes and black branes
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• Quasinormal modes of black holes: from astrophysics to string theory
• f(T) teleparallel gravity and cosmology
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
• Interferometer design of the KAGRA gravitational wave detector
• A gravitational wave observatory operating beyond the quantum shot-noise limit: Squeezed light in application
• Challenges for $\Lambda$CDM: An update
• Gravitational-wave sensitivity curves
• A simple model of complete precessing black-hole-binary gravitational waveforms
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations
• Binary neutron-star mergers: a review of Einstein's richest laboratory
• I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics
• Squeezed states of light and their applications in laser interferometers
• Detection methods for stochastic gravitational-wave backgrounds: a unified treatment
• The Evolution of Compact Binary Star Systems
• The Effective Field Theorist's Approach to Gravitational Dynamics
• Gravitational Waves Induced by non-Gaussian Scalar Perturbations
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Quantum Metrology for Gravitational Wave Astronomy
• Dynamical Mass Ejection from Binary Neutron Star Mergers
• A Cosmological Signature of the SM Higgs Instability: Gravitational Waves
• Approximate Universal Relations for Neutron Stars and Quark Stars
• Systematic parameter errors in inspiraling neutron star binaries
• A New Method for Gravitational Wave Detection with Atomic Sensors
• Constraining the Equation of State of Neutron Stars from Binary Mergers
• Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
• Networks of gravitational wave detectors and three figures of merit
• Testing strong-field gravity with tidal Love numbers
• NANOGrav Hints to Primordial Black Holes as Dark Matter
• Possible Indirect Confirmation of the Existence of Pop III Massive Stars by Gravitational Wave
• Deep Neural Networks to Enable Real-time Multimessenger Astrophysics
• Gravitational Radiation Detection with Laser Interferometry
• The origins of massive black holes
• The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope
• Expected properties of the first gravitational wave signal detected with pulsar timing arrays
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• Modified theories of Gravity: Why, How and What?
• Gravitational waves induced by scalar perturbations as probes of the small-scale primordial spectrum
• Gravitational waves from neutron stars: Promises and challenges
• The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes
• Cosmology with the lights off: Standard sirens in the Einstein Telescope era
• Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
• Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
• Circumbinary MHD Accretion into Inspiraling Binary Black Holes
• Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae
• Bayesian model selection for testing the no-hair theorem with black hole ringdowns
• Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation
• Primordial black holes and second order gravitational waves from ultra-slow-roll inflation
• A Xylophone Configuration for a third Generation Gravitational Wave Detector
• Generating PBHs and small-scale GWs in two-field models of inflation
• Fast and Accurate Inference on Gravitational Waves from Precessing Compact Binaries
• Glitch Classification and Clustering for LIGO with Deep Transfer Learning
• Deep Transfer Learning: A new deep learning glitch classification method for advanced LIGO
• Multiband Gravitational-Wave Astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO
• Massive binary black holes in galactic nuclei and their path to coalescence
• Tracking the precession of compact binaries from their gravitational-wave signal
• Gravitational wave signatures of the absence of an event horizon. I. Nonradial oscillations of a thin-shell gravastar
• Gravitational-wave Limits from Pulsar Timing Constrain Supermassive Black Hole Evolution
• Beyond second-order convergence in simulations of binary neutron stars in full general-relativity
• Gravitational Wave Production right after a Primordial Black Hole Evaporation
• Compact binary systems in scalar-tensor gravity: Equations of motion to 2.5 post-Newtonian order
• Primordial gravitational waves from NANOGrav: a broken power-law approach
• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• The Gravitational-Wave Physics
• Induced gravitational waves in a general cosmological background
• Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network
• Gravitational and electromagnetic outputs from binary neutron star mergers
• Precision cosmology from future lensed gravitational wave and electromagnetic signals
• Next to leading order spin-orbit effects in the motion of inspiralling compact binaries
• Comparing Equivalent Gravities: common features and differences
• Double inflation as a single origin of primordial black holes for all dark matter and LIGO observations
• Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era
• The electromagnetic counterparts of compact binary mergers
• Editorial for the Special Issue 100 Years of Chronogeometrodynamics: The Status of the Einstein's Theory of Gravitation in Its Centennial Year
• Enhancement of Gravitational Waves Induced by Scalar Perturbations due to a Sudden Transition from an Early Matter Era to the Radiation Era
• Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation
• The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
• No further gravitational wave modes in $F(T)$ gravity
• Probing Extreme-Density Matter with Gravitational Wave Observations of Binary Neutron Star Merger Remnants
• On the gravitational wave background from compact binary coalescences in the band of ground-based interferometers
• The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range
• Geometrical Expression for the Angular Resolution of a Network of Gravitational-Wave Detectors
• Effects of waveform model systematics on the interpretation of GW150914
• Fundamentals of the orbit and response for TianQin
• A Resonant Mode for Gravitational Wave Detectors based on Atom Interferometry
• Phase effects from strong gravitational lensing of gravitational waves
• Complete waveform model for compact binaries on eccentric orbits
• Searches for Continuous-Wave Gravitational Radiation
• Distance measures in gravitational-wave astrophysics and cosmology
• Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
• Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
• Finding the chiral gravitational wave background of an axion-SU(2) inflationary model using CMB observations and laser interferometers
• Constraints on Binary Black Hole Populations from LIGO-Virgo Detections
• Improving the sensitivity of a search for coalescing binary black holes with non-precessing spins in gravitational wave data
• Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters
• Gravitational Waves from Collapsing Domain Walls
• Black hole-neutron star binary merger: Dependence on black hole spin orientation and equations of state
• The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse
• Gravitational Waves: Sources, Detectors and Searches
• Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
• Perturbations of Schwarzschild black holes in Dynamical Chern-Simons modified gravity
• Frequency and time domain inspiral templates for comparable mass compact binaries in eccentric orbits
• Testing General Relativity using Bayesian model selection: Applications to observations of gravitational waves from compact binary systems
• Constraints on primordial density perturbations from induced gravitational waves
• Correlated Signatures of Gravitational-Wave and Neutrino Emission in Three-Dimensional General-Relativistic Core-Collapse Supernova Simulations
• Subtraction of Newtonian Noise Using Optimized Sensor Arrays
• Gravitational waves from oscillons after inflation
• Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond
• Waveform of gravitational waves in the general parity-violating gravities
• Derivation of local-in-time fourth post-Newtonian ADM Hamiltonian for spinless compact binaries
• The One-Armed Spiral Instability in Neutron Star Mergers and its Detectability in Gravitational Waves
• Multipole Love Relations
• Kadath: a spectral solver for theoretical physics
• ASTROD-GW: Overview and Progress
• Lunar Gravitational-Wave Antenna
• Parameter estimation with gravitational waves
• The Overlap of Numerical Relativity, Perturbation Theory and Post-Newtonian Theory in the Binary Black Hole Problem
• Dark stars: gravitational and electromagnetic observables
• Mining Gravitational-wave Catalogs To Understand Binary Stellar Evolution: A New Hierarchical Bayesian Framework
• Review of the Advanced LIGO gravitational wave observatories leading to observing run four
• Quasinormal mode oscillations in an analogue black hole experiment
• Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo
• Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
• A high-flux BEC source for mobile atom interferometers
• Multimessenger astronomy with gravitational waves and high-energy neutrinos
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• The Initial Value Formulation of Dynamical Chern-Simons Gravity
• Narrow double-peaked emission lines of SDSS J131642.90+175332.5: signature of a single or a binary AGN in a merger, jet-cloud interaction, or unusual narrow-line region geometry
• Primordial black hole tower: Dark matter, earth-mass, and LIGO black holes
• Vacuum Electromagnetic Counterparts of Binary Black-Hole Mergers
• Binary black hole coalescence in the large-mass-ratio limit: the hyperboloidal layer method and waveforms at null infinity
• Bounding the mass of the graviton with gravitational waves: Effect of higher harmonics in gravitational waveform templates
• Canonical Formulation of Spin in General Relativity
• Gravitational wave spectroscopy of binary neutron star merger remnants with mode stacking
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• Cosmological inference using only gravitational wave observations of binary neutron stars
• Gravitational waves from the minimal gauged $U(1{)}_{B-L}$ model
• Are gravitational waves from giant magnetar flares observable?
• The numerical relativity breakthrough for binary black holes
• GRMHD simulations of prompt-collapse neutron star mergers: the absence of jets
• Effect of calibration errors on Bayesian parameter estimation for gravitational wave signals from inspiral binary systems in the advanced detectors era
• Spectrum of Primordial Gravitational Waves in Modified Gravities: A Short Overview
• Effects of nonquadrupole modes in the detection and parameter estimation of black hole binaries with nonprecessing spins
• LISA Sensitivities to Gravitational Waves from Relativistic Metric Theories of Gravity
• Scientific Potential of DECIGO Pathfinder and Testing GR with Space-Borne Gravitational Wave Interferometers
• Gravitational Wave Polarization Modes in $f(R)$ Theories
• Constraining the time variation of Newton's constant $G$ with gravitational-wave standard sirens and supernovae
• Binary Black Hole Mergers from LIGO/Virgo O1 and O2: Population Inference Combining Confident and Marginal Events
• Constraints on primordial curvature perturbations from primordial black hole dark matter and secondary gravitational waves
• Testing Brans-Dicke gravity using the Einstein telescope
• Gravitational waves at the first post-Newtonian order with the Weyssenhoff fluid in Einstein-Cartan theory
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• Observing gravitational wave bursts in pulsar timing measurements
• Tidal deformability of dressed black holes and tests of ultralight bosons in extended mass ranges
• First Law of Mechanics for Compact Binaries on Eccentric Orbits
• Fermi-LAT Observations of the LIGO event GW150914
• Gravitational properties of light - The gravitational field of a laser pulse
• White dwarfs stripped by massive black holes: sources of coincident gravitational and electromagnetic radiation
• New pulsar limit on local Lorentz invariance violation of gravity in the standard-model extension
• GWFish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks
• Applying deep neural networks to the detection and space parameter estimation of compact binary coalescence with a network of gravitational wave detectors
• Gravitational-wave signatures of the absence of an event horizon. II. Extreme mass ratio inspirals in the spacetime of a thin-shell gravastar
• Template banks to search for low-mass binary black holes in advanced gravitational-wave detectors
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Linking electromagnetic and gravitational radiation in coalescing binary neutron stars
• Constraining the mass of the graviton using coalescing black-hole binaries
• Systematic bias on parameterized tests of general relativity due to neglect of orbital eccentricity
• On the Solution Space of Differentially Rotating Neutron Stars in General Relativity
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• Probing mass-radius relation of protoneutron stars from gravitational-wave asteroseismology
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• The NINJA-2 project: Detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations
• Conversion of relic gravitational waves into photons in cosmological magnetic fields
• Probing modified gravity theories and cosmology using gravitational-waves and associated electromagnetic counterparts
• Neutron stars versus black holes: probing the mass gap with LIGO/Virgo
• Gravitational wave sources in the era of multi-frequency gravitational wave astronomy
• Waveform of gravitational waves in the ghost-free parity-violating gravities
• Towards the Design of Gravitational-Wave Detectors for Probing Neutron-Star Physics
• Strongly Lensed Transient Sources: A Review
• Probing Gravitational Parity Violation with Gravitational Waves from Stellar-mass Black Hole Binaries
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Constraining the equation of state of nuclear matter with gravitational wave observations: Tidal deformability and tidal disruption
• Gravitational Wave Astronomy With TianQin
• Model-independent test of gravity with a network of ground-based gravitational-wave detectors
• Gravitational wave detection in space
• Probing the seesaw scale with gravitational waves
• Impact of high-order tidal terms on binary neutron-star waveforms
• Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing run
• General treatment of quantum and classical spinning particles in external fields
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Accuracy of gravitational waveform models for observing neutron-star--black-hole binaries in Advanced LIGO
• Testing the multipole structure of compact binaries using gravitational wave observations
• Breaking the mass-sheet degeneracy with gravitational wave interference in lensed events
• Probing Cosmic Superstrings with Gravitational Waves
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Propagation of Gravitational Waves in Generalized TeVeS
• Primordial Gravitational Waves Predictions for GW170817-compatible Einstein-Gauss-Bonnet Theory
• Denoising of gravitational wave signals via dictionary learning algorithms
• Astro2010 Decadal Survey Whitepaper: Coordinated Science in the Gravitational and Electromagnetic Skies
• Neutron star tidal disruption in mixed binaries: the imprint of the equation of state
• Dark energy, co-evolution of massive black holes with galaxies, and ASTROD-GW
• Reliability of complete gravitational waveform models for compact binary coalescences
• Quasinormal frequencies of self-dual black holes
• Afterglow constraints on the viewing angle of binary neutron star mergers and determination of the Hubble constant
• Constraints on the Nieh-Yan modified teleparallel gravity with gravitational waves
• Stochastic gravitational wave background from hydrodynamic turbulence in differentially rotating neutron stars
• Impact of eccentricity on the gravitational wave searches for binary black holes: High mass case
• Numerical simulations of stellar collapse in scalar-tensor theories of gravity
• Generalized quasi-Keplerian solution for eccentric, non-spinning compact binaries at 4PN order and the associated IMR waveform
• Testing general relativity with gravitational waves: a reality check
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Observing the Galaxy's massive black hole with gravitational wave bursts
• On the identification of individual gravitational wave image types of a lensed system using higher-order modes
• Gravitational waves from axion-like particle cosmic string-wall networks
• Detectability of thermal neutrinos from binary-neutron-star mergers and implication to neutrino physics
• Detection of astrophysical gravitational wave sources by TianQin and LISA
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Tests of gravitational symmetries with radio pulsars
• Tests of general relativity using multiband observations of intermediate mass binary black hole mergers
• Exploring the Spectral Shape of Gravitational Waves Induced by Primordial Scalar Perturbations and Connection with the Primordial Black Hole Scenarios
• Noisy neighbours: inference biases from overlapping gravitational-wave signals
• Novel Method for Incorporating Model Uncertainties into Gravitational Wave Parameter Estimates
• Gravitational Wave Memory: A New Approach to Study Modified Gravity
• Improvements to the construction of binary black hole initial data
• Small scale induced gravitational waves from primordial black holes, a stringent lower mass bound, and the imprints of an early matter to radiation transition
• Testing the validity of the single-spin approximation in inspiral-merger-ringdown waveforms
• Light scalar field constraints from gravitational-wave observations of compact binaries
• Coherent Network Analysis of Gravitational Waves from Three-Dimensional Core-Collapse Supernova Models
• physiCal: A physical approach to the marginalization of LIGO calibration uncertainties
• Catastrogenesis: DM, GWs, and PBHs from ALP string-wall networks
• Detection of Gravitational Waves Using Bayesian Neural Networks
• Testing the Etherington's distance duality relation at higher redshifts: the combination of radio quasars and gravitational waves
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Frequency response of space-based interferometric gravitational-wave detectors
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Multiband gravitational-wave searches for ultralight bosons
• Continuous gravitational wave from magnetized white dwarfs and neutron stars: possible missions for LISA, DECIGO, BBO, ET detectors
• Measuring the delay time distribution of binary neutron stars. II. Using the redshift distribution from third-generation gravitational wave detectors network
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• Lattice template placement for coherent all-sky searches for gravitational-wave pulsars
• Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
• Cosmology with Gravitational Wave/Fast Radio Burst Associations
• Gravitational waves in Poincaré gauge gravity theory
• Astronomical Distance Determination in the Space Age. Secondary distance indicators
• Hubble parameter estimation via dark sirens with the LISA-Taiji network
• Measuring neutron star tidal deformability with Advanced LIGO: a Bayesian analysis of neutron star - black hole binary observations
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Tilted torus magnetic fields in neutron stars and their gravitational wave signatures
• Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes
• Multimessenger Search for Sources of Gravitational Waves and High-Energy Neutrinos: Results for Initial LIGO-Virgo and IceCube
• Gravitational Waves and Primordial Black Holes from Supersymmetric Hybrid Inflation
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Weak Gravitational Field in Finsler-Randers Space and Raychaudhuri Equation
• When black holes collide: Probing the interior composition by the spectrum of ringdown modes and emitted gravitational waves
• Oscillons from Pure Natural Inflation
• Viewing angle of binary neutron star mergers
• How current loops and solenoids curve space-time
• Detecting the Beaming Effect of Gravitational Waves
• Testing Brans-Dicke Gravity with Screening by Scalar Gravitational Wave Memory
• Flat parameter-space metric for all-sky searches for gravitational-wave pulsars
• Increasing LIGO sensitivity by feedforward subtraction of auxiliary length control noise
• A coherent method for the detection and estimation of continuous gravitational wave signals using a pulsar timing array
• Radiative losses and radiation-reaction effects at the first post-Newtonian order in Einstein-Cartan theory
• Gravitational wave observations, distance measurement uncertainties, and cosmology
• Generic bounds on dipolar gravitational radiation from inspiralling compact binaries
• Detecting Accelerating Eccentric Binaries in the LISA Band
• Stochastic gravitational wave background: methods and Implications
• Sensitivity functions for space-borne gravitational wave detectors
• Generalized plane waves in Poincaré gauge theory of gravity
• Phenomenological Relations for Axial Quasi-normal Modes of Neutron Stars with Realistic Equations of State
• Gravitational-wave selection effects using neural-network classifiers
• Application of asymptotic expansions for maximum likelihood estimators' errors to gravitational waves from binary mergers: the network case
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• Total-variation-based methods for gravitational wave denoising
• Angular and frequency response of the gravitational wave interferometers in the metric theories of gravity
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Singular value decomposition in parametrised tests of post-Newtonian theory
• The case for testing MOND using LISA Pathfinder
• Exotic matter influence on the polar quasi-normal modes of neutron stars with equations of state satisfying the $2M_{\odot }$ constraint
• Initial data for neutron star binaries with arbitrary spins
• Analogue Black Hole Spectroscopy; or, how to listen to dumb holes
• Classical tests in brane gravity
• Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
• On the validity of the adiabatic approximation in compact binary inspirals
• Tests of General Relativity and Alternative theories of gravity using Gravitational Wave observations
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Estimating parameters of binary black holes from gravitational-wave observations of their inspiral, merger and ringdown
• Machine learning forecasts of the cosmic distance duality relation with strongly lensed gravitational wave events
• Observational upper limits on the gravitational wave production of core collapse supernovae
• Ready-to-use analytic model for gravitational waves from a hierarchical triple with Kozai-Lidov oscillations
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Circular polarization of gravitational waves from non-rotating supernova cores: a new probe into the pre-explosion hydrodynamics
• Gauge transformation of scalar induced tensor perturbation during matter domination
• A Linear and Quadratic Time-Frequency Analysis of Gravitational Waves from Core-Collapse Supernovae
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• The Zadko Telescope: A Southern Hemisphere Telescope for Optical Transient Searches, Multi-Messenger Astronomy and Education
• Gravitational waves, dark energy and inflation
• Detecting relics of a thermal gravitational wave background in the early Universe
• Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity
• Collapse of differentially rotating supermassive stars: Post black hole formation
• Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Clocks around Sgr A*
• Multivariate Classification with Random Forests for Gravitational Wave Searches of Black Hole Binary Coalescence
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• Reduced Order and Surrogate Models for Gravitational Waves
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits
• Towards establishing the presence or absence of horizons in coalescing binaries of compact objects by using their gravitational wave signals
• The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Total-variation methods for gravitational-wave denoising: performance tests on Advanced LIGO data
• Characterization of binary black holes by heterogeneous gravitational-wave networks
• Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors
• Dressing the Post-Newtonian two-body problem and Classical Effective Field Theory
• Optimal estimation of time-dependent gravitational fields with quantum optomechanical systems
• The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
• Resonant Dampers for Parametric Instabilities in Gravitational Wave Detectors
• Limits on high-frequency gravitational wave background from its interplay with large scale magnetic fields
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short $\gamma$-ray bursts
• Timescales for detection of super-Chandrasekhar white dwarfs by gravitational wave astronomy
• Testing quasilinear modified Newtonian dynamics in the Solar System
• Synergy of short gamma ray burst and gravitational wave observations: Constraining the inclination angle of the binary and possible implications for off-axis gamma ray bursts
• Discovering the interior of black holes
• Observing binary black hole ringdowns by advanced gravitational wave detectors
• Millisecond Magnetars
• Massive Black Hole Science with eLISA
• Mergers of black hole-neutron star binaries and rates of associated electromagnetic counterparts
• Sensitivity of Space-based Gravitational-Wave Interferometers to Ultralight Bosonic Fields and Dark Matter
• Nanohertz Gravitational Wave Astronomy during the SKA Era: An InPTA perspective
• Third-and-a-half order post-Newtonian equations of motion for relativistic compact binaries using the strong field point particle limit
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Amplification of the Primordial Gravitational Waves Energy Spectrum by a Kinetic Scalar in $F(R)$ Gravity
• Convergence of Fourier-domain templates for inspiraling eccentric compact binaries
• Gravitational wave in f(R) gravity: possible signature of sub- and super-Chandrasekhar limiting mass white dwarfs
• Resonant high energy graviton to photon conversion at post recombination epoch
• Leading-order spin-orbit and spin(1)-spin(2) radiation-reaction Hamiltonians
• Searching for near-horizon quantum structures in the binary black-hole stochastic gravitational-wave background
• Constraining the propagation speed of gravitational waves with compact binaries at cosmological distances
• Binary Black Hole Waveform Extraction at Null Infinity
• The Final Merger of Black-Hole Binaries
• Bound on Induced Gravitational Waves during Inflation Era
• Tetrads in SU(N) Yang-Mills geometrodynamics
• Orbital effects on time delay interferometry for TianQin
• Up to eleven: radiation from particles with arbitrary energy falling into higher-dimensional black holes
• Distinguishing general relativity from Chern-Simons gravity using gravitational wave polarizations
• Scalar Gravitational Waves in the Effective Theory of Gravity
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Fake massive black holes in the milli-Hertz gravitational-wave band
• On the equal-mass limit of precessing black-hole binaries
• Facilitating follow-up of LIGO-Virgo events using rapid sky localization
• Use of Excess Power Method and Convolutional Neural Network in All-Sky Search for Continuous Gravitational Waves
• Amplification of Primordial Gravitational Waves by a Geometrically Driven non-canonical Reheating Era
• Induced gravitational waves: the effect of first order tensor perturbations
• Prospects for multi-messenger extended emission from core-collapse supernovae in the Local Universe
• Identifying Host Galaxies of Supermassive Black Hole Binaries Found by PTAs
• Domain Walls and Gravitational Waves after Thermal Inflation
• Anisotropic multimessenger signals from black hole neutrino-dominated accretion flows with outflows in binary compact object mergers
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds
• Signatures of a High Temperature QCD Transition in the Early Universe
• Unbiased Cosmic Opacity Constraints from Standard Sirens and Candles
• $f(R)$-Gravity Generated Post-inflationary Eras and their Effect on Primordial Gravitational Waves
• Future Gravitational Wave Detectors Based on Atom Interferometry
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Gravitational waves and electrodynamics: New perspectives
• Stochastic gravitational wave background from magnetic deformation of newly born magnetars
• Degeneracy between mass and peculiar acceleration for the double white dwarfs in the LISA band
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• Nearby stars as gravitational wave detectors
• An axion-like scalar field environment effect on binary black hole merger
• Polarization Modes of Gravitational Wave for Viable f(R) Models
• Effects of a Pre-inflationary de Sitter Bounce on the Primordial Gravitational Waves in $f(R)$ Gravity Theories
• Parity violation in gravitational waves and observational bounds from third-generation detectors
• Testing gravity with gravitational wave friction and gravitational slip
• Upper limits on persistent gravitational waves using folded data and the full covariance matrix from Advanced LIGO${}^{\prime }$s first two observing runs
• Strategies for the Follow-up of Gravitational Wave Transients with the Cherenkov Telescope Array
• Gravitational Waves from Peaks
• The cross-correlation search for a hot spot of gravitational waves
• How photon astronomy affects searches for continuous gravitational waves
• Stochastic gravitational wave background from newly born massive magnetars: The role of a dense matter equation of state
• Rapidly rotating neutron star progenitors
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Hierarchical approach to matched filtering using a reduced basis
• Torsional oscillations of crystalline color-superconducting hybrid stars: Possible sources for Advanced LIGO?
• Complex orbital dynamics of a double neutron star system revolving around a massive black hole
• Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
• Mapping the shape of the scalar potential with gravitational waves
• Strong gravity signatures in the polarization of gravitational waves
• The stochastic background of gravitational waves due to the f-mode instability in neutron stars
• Memory-triggered supernova neutrino detection
• Effect of squeezing on parameter estimation of gravitational waves emitted by compact binary systems
• Strongly lensed gravitational waves as the probes to test the cosmic distance duality relation
• Exploring the CPT violation and birefringence of gravitational waves with ground- and space-based gravitational-wave interferometers
• Characterization of low-significance gravitational-wave compact binary sources
• Exploring departures from Schwarzschild black hole in $f(R)$ gravity
• Method for estimation of gravitational-wave transient model parameters in frequency-time maps
• Response of a spaceborne gravitational wave antenna to solar oscillations
• Atick-Witten Hagedorn Conjecture, near scale-invariant matter and blue-tilted gravity power spectrum
• Scalar self-force for eccentric orbits around a Schwarzschild black hole
• ADC non-linear errors correction in thermal diagnostics for the LISA mission
• Probing Stochastic Ultralight Dark Matter with Space-based Gravitational-Wave Interferometers
• Python Open Source Waveform Extractor (POWER): An open source, Python package to monitor and post-process numerical relativity simulations
• Gravitational waves in metric-affine gravity theory
• Bayesian inference for binary neutron star inspirals using a Hamiltonian Monte Carlo Algorithm
• On the gauge dependence of scalar induced secondary gravitational waves during radiation and matter domination eras
• On the weight of entanglement
• Gravitational Waves from Incomplete Inflationary Phase Transitions
• Swarm-intelligent search for gravitational waves from eccentric binary mergers
• Quantum gravitational signatures in next-generation gravitational wave detectors
• Testing the anisotropy of the universe using the simulated gravitational wave events from advanced LIGO and Virgo
• Impact of unmodeled eccentricity on the tidal deformability measurement and implications for gravitational wave physics inference
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
• Ballistic orbits in Schwarzschild space-time and gravitational waves from EMR binary mergers
• Parametrized tests of general relativity using eccentric compact binaries
• The rise of the primordial tensor spectrum from an early scalar-tensor epoch
• Parameter estimates in binary black hole collisions using neural networks
• Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
• Detection of gravitational waves in circular particle accelerators
• Initial Conditions for Numerical Relativity -- Introduction to numerical methods for solving elliptic PDEs
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• Quadrupolar power radiation by a binary system in de Sitter Background
• The First Detection of Gravitational Waves
• Numerical evolution of general Robinson-Trautman spacetimes: code tests, wave forms and the efficiency of the gravitational wave extraction
• Thermodynamics of relativistic quantum fields confined in cavities
• Identification of long-duration noise transients in LIGO and Virgo
• Octahedron configuration for a displacement noise-cancelling gravitational wave detector in space
• Estimation of the gravitational wave polarizations from a non template search
• Astronomy and astrophysics with gravitational waves in the Advanced Detector Era
• Obtaining Gravitational Waves from Inspiral Binary Systems using LIGO data
• Gravitational memory signal from neutrino self-interactions in supernova
• Quantum spacetime fluctuations: Lamb Shift and hyperfine structure of the hydrogen atom
• A Rømer time-delay determination of the gravitational-wave propagation speed
• Gravitational Waves from Direct Collapse Black Holes Formation
• The appearance of a merging binary black hole very close to a spinning supermassive black hole
• Model-independent measurement of the absolute magnitude of Type Ia Supernovae with gravitational-wave sources
• Measuring the maximally allowed polarization states of the isotropic stochastic gravitational wave background with the ground-based detectors
• Mission Design for the TAIJI misson and Structure Formation in Early Universe
• Augmented kludge waveforms and Gaussian process regression for EMRI data analysis
• Cylindrically symmetric inhomogeneous dust collapse with a zero expansion component
• How to confirm the existence of population III stars by observations of gravitational waves
• Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• Gravitational radiation by magnetic field: application to millisecond magnetars
• Distortion of Gravitational-wave Signals by Astrophysical Environments
• Template-space metric for searches for gravitational waves from the inspiral, merger and ringdown of binary black holes
• Luminosity distance uncertainties from gravitational wave detections by third generation observatories
• Mass and tidal parameter extraction from gravitational waves of binary neutron stars mergers using deep learning
• Forecasting Gamma-Ray Bursts using Gravitational Waves
• Global Optimization for Future Gravitational Wave Detectors' Sites
• Origin of the Chemical Elements
• Interaction between gravitational radiation and electromagnetic radiation
• Scalar and Fermion field interactions with a gravitational wave
• Relativistic scattering of a fast spinning neutron star by a massive black hole
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Stochastic Gravitational Wave Background from Exoplanets
• Calibration of the in-orbit center-of-mass of TaiJi-1
• Extended Geometric Trinity of Gravity
• The attribute of rotational profile to the hyperon puzzle in the prediction of heaviest compact star
• Deep Learning for estimating parameters of Gravitational Waves
• Scalar Stochastic Gravitational-Wave Background in Brans-Dicke Theory of Gravity
• An exact model for evaporating primordial black holes in cosmological space-time
• Effects of vertical advection on multimessenger signatures of black hole neutrino-dominated accretion flows in compact binary coalescences
• Bursts of Gravitational Waves due to Crustquake from Pulsars
• Fast prediction and evaluation of eccentric inspirals using reduced-order models
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Measuring the speed of light with cosmological observations: current constraints and forecasts
• A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
• The Indian Pulsar Timing Array Data Release 2: I. Dataset and Timing Analysis
• Fast Radio Bursts signal high-frequency gravitational waves
• Low latency search for Gravitational waves from BH-NS binaries in coincidence with Short Gamma Ray Bursts
• High frequency background gravitational waves from spontaneous emission of gravitons by hydrogen and helium
• The energy spectrum of gravitational waves in a loop quantum cosmological model
• Gravito-electromagnetic resonances in Minkowski space
• Propagation of gravitational waves in multimetric gravity
• Stochastic microhertz gravitational radiation from stellar convection
• A new estimation method for mass of an isolated neutron star using gravitational waves
• Numerical relativity simulations in the era of the Einstein Telescope
• Optical Detector Topology for Third-Generation Gravitational Wave Observatories
• Dynamic black holes through gravitational collapse: Analysis of multipole moment of the curvatures on the horizon
• Ground-state Wigner functional of linearized gravitational field
• The Distributional Stress-Energy Quadrupole
• Compact star deformation and universal relationship for magnetized white dwarfs
• Electromagnetic memory in arbitrary curved space-times
• Probing the formation of the seeds of supermassive black holes with gravitational waves
• Multipolar Particles in Helically Symmetric Spacetimes
• Advanced technologies for future ground-based, laser-interferometric gravitational wave detectors
• Imprints of massive black-hole binaries on neighbouring decihertz gravitational-wave sources
• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars
• Imprints of extra dimensions in eccentric extreme-mass-ratio inspirals gravitational waveforms
• Probability distribution function for inclinations of merging compact binaries detected by gravitational wave interferometers
• Search for an emission line of a gravitational wave background
• On the initial spin periods of magnetars born in weak supernova explosions and their gravitational wave radiation
• Cosmology in the dark: How compact binaries formation impact the gravitational-waves cosmological measurements
• How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
• Interferometer Euro-Asian Network: Detection Characteristics for Signals of Known Shape
• The LOFT mission: new perspectives in the research field of (accreting) compact objects
• Stochastic gravitational wave background from accreting primordial black hole binaries during early inspiral stage
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
• Post-newtonian analysis of precessing convention for spinning compact binaries
• Extreme mass-ratio inspirals and extra dimensions: Insights from modified Teukolsky framework
• Distinguishing Monochromatic Signals in LISA and Taiji: Ultralight Dark Matter versus Gravitational Waves
• Probing the Dark Solar System: Detecting Binary Asteroids with a Space-Based Interferometric Asteroid Explorer
• On non-detection of Gamma-Ray Bursts in three compact binary merger events detected by LIGO
• Eccentric Pairs: Analytic Gravitational Waves from Binary Black Holes in Elliptic Orbits
• Orbital effects of a monochromatic plane gravitational wave with ultra-low frequency incident on a gravitationally bound two-body system
• Electromagnetic signatures of far-field gravitational radiation in the 1+3 approach
• Quantization of the nonstandard propagating gravitational waves in the cosmological background
• Interpreting gravitational-wave burst detections: constraining source properties without astrophysical models
• Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors
• Merging Black Holes: Assessing the Performance of Two Analytic Gravitational Waves Models
• First joint observation by the underground gravitational-wave detector, KAGRA, with GEO600
• Gravito-optics and intensity correlations for binary inspiral signal detections
• Deriving Neutron Star Equation of State from AdS/QCD
• Sensing and vetoing loud transient noises for the gravitational-wave detection
• Beyond the Long Wavelength Approximation: Next-generation Gravitational-Wave Detectors and Frequency-dependent Antenna Patterns
• Unified laboratory-frame analysis of atomic gravitational-wave sensors
• Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions
• On the occurrence of gauge-dependent secularities in nonlinear gravitational waves
• Transient electromagnetic sources can detect solitary black holes in Milky Way galaxy
• Reduced order modelling in searches for continuous gravitational waves - I. Barycentering time delays
• Detecting milli-Hz gravitational waves with optical resonators
• Spacetime Symmetries and Kepler's Third Law
• The constraints on the stochastic gravitational wave background from cosmic strings by an electromagnetic resonance system
• Cosmological perturbations in the energy-momentum squared gravity theory: constraints from gravitational wave standard sirens and redshift space distortions
• A 1+5-dimensional gravitational-wave solution: curvature singularity and spacetime singularity
• Tidal reconstruction of neutron star mergers from their late inspiral
• Imprints of the redshift evolution of double neutron star merger rate on the signal to noise ratio distribution
• The Emission of Electromagnetic Radiation from Charges Accelerated by Gravitational Waves and its Astrophysical Implications
• The road to gravitational-wave astronomy
• Data Analysis Methods for Testing Alternative Theories of Gravity with LISA Pathfinder
• Could the stochastic gravitational wave background from newborn magnetars be detected by the advanced LIGO and Einstein Telescope?
• Absorption and scattering of massless scalar waves by Frolov black holes
• Tests of Modified Gravity Theories in the Solar System
• Generation of gravitating solutions with Baryonic charge from Einstein-Scalar-Maxwell seeds
• Master Functions and Equations for Perturbations of Vacuum Spherically-Symmetric Spacetimes
• The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries
• Non-analytical power law correction to the Einstein-Hilbert action: gravitational wave propagation
• Gravitational-wave echoes from spinning exotic compact objects: numerical waveforms from the Teukolsky equation
• Coherent versus coincidence detection of gravitational wave signals from compact inspiraling binaries
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Black-hole ringdown with templates capturing spin precession: A reanalysis of GW190521
• Primordial black holes from D-parity breaking in SO(10) grand unified theory
• Population Properties of Binary Black Holes with Eccentricity
• Searching for gravitational waves from compact binary mergers powering long gamma-ray bursts during LIGO-Virgo-KAGRA's O3 run
• High Sensitivity Methodologies to Detect Radio Band Gravitational Waves
• Tests of scalar polarizations with multi-messenger events
• Impact and detectability of spin-tidal couplings in neutron star inspirals
• Mass flow in the circumbinary disk with gap around supermassive binary black holes
• Timescales for Detecting Magnetized White Dwarfs in Gravitational Wave Astronomy
• Gravitational wave signature of a mini creation event (MCE)
• Coincidence searches of gravitational waves and short gamma-ray bursts
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• Detecting stochastic gravitational wave background from cosmic strings with next-generation detector networks: Component separation based on a multi-source astrophysical foreground noise model
• Source Confusion of Massive Black Hole Binaries for the Taiji Mission
• Time-domain inspiral templates for spinning compact binaries in quasi-circular orbits
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Inspiral waveforms for spinning compact binaries in a new precessing convention
• Graph-based Summary Statistics for Revealing the Stochastic Gravitational Wave Background in Pulsar Timing Arrays
• Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
• A Novel Search Technique for Low-Frequency Periodic Gravitational Waves
• The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
• Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range