Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian order

Abstract

The rate of gravitational-wave energy loss from inspiralling binary systems of compact objects of arbitrary mass is derived through second post-Newtonian (2PN) order $O[(Gm/r{c}^2{)}^2]$ beyond the quadrupole approximation. The result has been derived by two independent calculations of the (source) multipole moments. The 2PN terms, and in particular the finite mass contribution therein (which cannot be obtained in perturbation calculations of black hole spacetimes), are shown to make a significant contribution to the accumulated phase of theoretical templates to be used in matched filtering of the data from future gravitational-wave detectors.

12 pages, RevTeX 3.0. Direct all correspondence to [email protected], FAX 314-935-6219

References in corpus (3)

• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Testing Scalar-Tensor Gravity with Gravitational-Wave Observations of Inspiralling Compact Binaries
• Second-post-Newtonian generation of gravitational radiation

Cited by in corpus (355)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The Confrontation between General Relativity and Experiment
• Multi-messenger Observations of a Binary Neutron Star Merger
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• 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
• GW170817: Measurements of Neutron Star Radii and Equation of State
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• The Confrontation between General Relativity and Experiment
• Effective one-body approach to general relativistic two-body dynamics
• Properties of the binary neutron star merger GW170817
• LIGO: The Laser Interferometer Gravitational-Wave Observatory
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space
• Physics, Astrophysics and Cosmology with Gravitational Waves
• Transition from inspiral to plunge in binary black hole coalescences
• Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
• Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
• Coalescing binary systems of compact objects to (post)$^{5/2}-Newtonian order. V. Spin Effects
• An Effective Field Theory of Gravity for Extended Objects
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
• Coalescence of Two Spinning Black Holes: An Effective One-Body Approach
• Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
• FINDCHIRP: an algorithm for detection of gravitational waves from inspiraling compact binaries
• Tests of General Relativity with GW170817
• The Confrontation between General Relativity and Experiment
• Search templates for gravitational waves from inspiraling binaries: Choice of template spacing
• Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
• GW150914: First results from the search for binary black hole coalescence with Advanced LIGO
• Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue
• Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals
• Matched filtering of gravitational waves from inspiraling compact binaries: Computational cost and template placement
• Exploring short gamma-ray bursts as gravitational-wave standard sirens
• Estimating spinning binary parameters and testing alternative theories of gravity with LISA
• A chi-squared time-frequency discriminator for gravitational wave detection
• Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order
• Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order
• Analytic black hole perturbation approach to gravitational radiation
• Gravitational radiation from compact binary systems: gravitational waveforms and energy loss to second post-Newtonian order
• Higher-order spin effects in the amplitude and phase of gravitational waveforms emitted by inspiraling compact binaries: Ready-to-use gravitational waveforms
• Improved filters for gravitational waves from inspiralling compact binaries
• The Progenitors of Short Gamma-Ray Bursts
• The evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission
• Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors
• A Comparison of search templates for gravitational waves from binary inspiral
• Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity. I. Method and tests
• Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit
• Gravitational-Wave Inspiral of Compact Binary Systems to 7/2 Post-Newtonian Order
• Gravitational waves from inspiraling compact binaries: The quadrupole-moment term
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence
• Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• Numerical Relativity and Compact Binaries
• Implementing a search for aligned-spin neutron star -- black hole systems with advanced ground based gravitational wave detectors
• Post-Newtonian Gravitational Radiation and Equations of Motion via Direct Integration of the Relaxed Einstein Equations. I. Foundations
• Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits
• Numerical Relativity: A review
• Search for Gravitational Waves from Low Mass Compact Binary Coalescence in LIGO's Sixth Science Run and Virgo's Science Runs 2 and 3
• Gravitational wave astronomy
• Getting a kick out of numerical relativity
• Gravitational waves from coalescing binaries: detection strategies and Monte Carlo estimation of parameters
• Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections
• Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
• Analysis of LIGO data for gravitational waves from binary neutron stars
• GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• LISA observations of rapidly spinning massive black hole binary systems
• Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation
• Measuring coalescing massive binary black holes with gravitational waves: The impact of spin-induced precession
• Gravitational waves from inspiralling compact binaries: Energy flux to third post-Newtonian order
• Phasing of gravitational waves from inspiralling eccentric binaries
• Radiative contribution to classical gravitational scattering at the third order in $G$
• Binary black-hole evolutions of excision and puncture data
• Comparing Effective-One-Body gravitational waveforms to accurate numerical data
• Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case
• The 2.5PN gravitational wave polarisations from inspiralling compact binaries in circular orbits
• Search for gravitational waves from binary inspirals in S3 and S4 LIGO data
• Dimensional regularization of the third post-Newtonian gravitational wave generation from two point masses
• Gravitational Wave Astronomy: in Anticipation of First Sources to be Detected
• Energy losses by gravitational radiation in inspiralling compact binaries to five halves post-Newtonian order
• Testing post-Newtonian theory with gravitational wave observations
• Dynamical invariants for general relativistic two-body systems at the third post-Newtonian approximation
• Probing the non-linear structure of general relativity with black hole binaries
• Spacetime structure near generic horizons and soft hair
• Measuring the parameters of massive black hole binary systems with Pulsar Timing Array observations of gravitational waves
• Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach
• Faithful Effective-One-Body waveforms of equal-mass coalescing black-hole binaries
• Detecting binary neutron star systems with spin in advanced gravitational-wave detectors
• Resonant Tidal Excitations of Rotating Neutron Stars in Coalescing Binaries
• Search for Gravitational Waves from Low Mass Binary Coalescences in the First Year of LIGO's S5 Data
• Using spin to understand the formation of LIGO's black holes
• Frequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binaries
• Self-interaction spin effects in inspiralling compact binaries
• Error-analysis and comparison to analytical models of numerical waveforms produced by the NRAR Collaboration
• Gravitational radiation reaction along general orbits in the effective one-body formalism
• Testing gravitational-wave searches with numerical relativity waveforms: Results from the first Numerical INJection Analysis (NINJA) project
• Third post-Newtonian angular momentum flux and the secular evolution of orbital elements for inspiralling compact binaries in quasi-elliptical orbits
• Higher signal harmonics, LISA's angular resolution, and dark energy
• On the equations of motion of point-particle binaries at the third post-Newtonian order
• Newtonian hydrodynamics of the coalescence of black holes with neutron stars IV: Irrotational binaries with a soft equation of state
• Tests of General Relativity with GWTC-3
• Accretion Processes On a Black Hole
• The Science Case for LIGO-India
• A data-analysis strategy for detecting gravitational-wave signals from inspiraling compact binaries with a network of laser-interferometric detectors
• Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3
• Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's first observing run
• Energy and angular momentum flow into a black hole in a binary
• Gravitational waves from a spinning particle in circular orbits around a rotating black hole
• Minding the gap: GW190521 as a straddling binary
• Gravitational radiation from a particle in circular orbit around a black hole. VI. Accuracy of the post-Newtonian expansion
• A template bank to search for gravitational waves from inspiralling compact binaries I: physical models
• Phasing of gravitational waves from inspiralling eccentric binaries at the third-and-a-half post-Newtonian order
• General Relativistic Models of Binary Neutron Stars in Quasiequilibrium
• On Estimation of the Post-Newtonian Parameters in the Gravitational-Wave Emission of a Coalescing Binary
• Testing General Relativity using Bayesian model selection: Applications to observations of gravitational waves from compact binary systems
• Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
• On the Progenitor of Binary Neutron Star Merger GW170817
• Binary Black Hole Mergers in 3d Numerical Relativity
• Parameterized Post-Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity
• A relativistic formalism to compute quasi-equilibrium configurations of non-synchronized neutron star binaries
• Detection Rate Estimates of Gravity-waves Emitted During Parabolic Encounters of Stellar Black Holes in Globular Clusters
• Coalescing Binary Neutron Stars
• Inadequacies of the Fisher Information Matrix in gravitational-wave parameter estimation
• The basic physics of the binary black hole merger GW150914
• A physical template family for gravitational waves from precessing binaries of spinning compact objects: Application to single-spin binaries
• Gravitational waveforms in scalar-tensor gravity at 2PN relative order
• Circular orbits of corotating binary black holes: comparison between analytical and numerical results
• Equations of Motion of Spinning Relativistic Particle in External Fields
• The Science of the Einstein Telescope
• Parameter estimation with gravitational waves
• Binary Neutron Stars in General Relativity: Quasi-Equilibrium Models
• Constraining alternative theories of gravity by gravitational waves from precessing eccentric compact binaries with LISA
• Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order
• Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity
• Gravitational radiation reaction and balance equations to post-Newtonian order
• Energy versus Angular Momentum in Black Hole Binaries
• Sub-second periodicity in a fast radio burst
• The curious case of GW200129: interplay between spin-precession inference and data-quality issues
• Binary black hole spectroscopy
• Mode coupling in the nonlinear response of black holes
• Searching for the full symphony of black hole binary mergers
• Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates
• Equation of motion for relativistic compact binaries with the strong field point particle limit : the second and half post-Newtonian order
• Dynamics of compact binary systems in scalar-tensor theories: I. Equations of motion to the third post-Newtonian order
• Investigating the effect of precession on searches for neutron-star-black-hole binaries with Advanced LIGO
• Effect of eccentricity on binary neutron star searches in Advanced LIGO
• The First Search for Gravitational Waves from Inspiraling Compact Binaries using TAMA300 data
• Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits
• Gravitational-Wave Phasing of Quasi-Circular Compact Binary Systems to the Fourth-and-a-Half post-Newtonian Order
• Tidal effects in the gravitational-wave phase evolution of compact binary systems to next-to-next-to-leading post-Newtonian order
• Bounding the mass of the graviton with gravitational waves: Effect of higher harmonics in gravitational waveform templates
• Bounding the mass of the graviton with gravitational waves: Effect of spin precessions in massive black hole binaries
• An early warning system for electromagnetic follow-up of gravitational-wave events
• Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning Compact Binaries to the Fourth Post-Newtonian Order
• Post-Newtonian expansion of gravitational waves from a particle in circular orbits around a rotating black hole: Up to $O(v^8)$ beyond the quadrupole formula
• Second post-Newtonian gravitational radiation reaction for two-body systems: Nonspinning bodies
• Localizing coalescing massive black hole binaries with gravitational waves
• Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order
• Scientific Potential of DECIGO Pathfinder and Testing GR with Space-Borne Gravitational Wave Interferometers
• A quasi-physical family of gravity-wave templates for precessing binaries of spinning compact objects: Application to double-spin precessing binaries
• LISA observations of supermassive black holes: parameter estimation using full post-Newtonian inspiral waveforms
• Innermost Stable Circular Orbit of Inspiraling Neutron-Star Binaries: Tidal Effects, Post-Newtonian Effects and the Neutron-Star Equation of State
• Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
• Time-dependence of the astrophysical stochastic gravitational wave background
• Search for subsolar-mass binaries in the first half of Advanced LIGO and Virgo's third observing run
• The dynamics of precessing binary black holes using the post-Newtonian approximation
• Equation of motion for relativistic compact binaries with the strong field point particle limit : Formulation, the first post-Newtonian and multipole terms
• First demonstration of early warning gravitational wave alerts
• Multiparameter tests of general relativity using multiband gravitational-wave observations
• Template banks to search for low-mass binary black holes in advanced gravitational-wave detectors
• Gravitational wave sources: reflections and echoes
• Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals
• Waveform systematics for binary neutron star gravitational wave signals: effects of the point-particle baseline and tidal descriptions
• Systematic bias on parameterized tests of general relativity due to neglect of orbital eccentricity
• NONLINEAR WAVE EQUATIONS FOR RELATIVITY
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence: Further investigations
• Gravitational-wave tail effects to quartic non-linear order
• Introductory lectures on the Effective One Body formalism
• Influence of conservative corrections on parameter estimation for extreme-mass-ratio inspirals
• Asymptotic gravitational wave fluxes from a spinning particle in circular equatorial orbits around a rotating black hole
• A geometric algorithm for efficient coincident detection of gravitational waves
• Gravitational waves from merging compact binaries
• 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
• Denoising of gravitational wave signals via dictionary learning algorithms
• Gravitational waves from inspiralling compact binaries with magnetic dipole moments
• Post-Newtonian Models of Binary Neutron Stars
• Testing General Relativity with Gravitational Waves: An Overview
• Higher harmonics increase LISA's mass reach for supermassive black holes
• Newtonian hydrodynamics of the coalescence of black holes with neutron stars III: Irrotational binaries with a stiff equation of state
• Targeted Sub-threshold Search for Strongly-lensed Gravitational-wave Events
• Relativistic orbits around spinning supermassive black holes. Secular evolution to 4.5 post-Newtonian order
• Testing Gravity with Gravitational Waves from Binary Black Hole Mergers: Contributions from Amplitude Corrections
• Tests of general relativity using multiband observations of intermediate mass binary black hole mergers
• Importance of including small body spin effects in the modelling of extreme and intermediate mass-ratio inspirals
• VAMANA: Modeling Binary Black Hole Population with Minimal Assumptions
• Template banks to search for compact binaries with spinning components in gravitational wave data
• Cross-correlation of the astrophysical gravitational-wave background with galaxy clustering
• Detecting gravitational waves from precessing binaries of spinning compact objects. II. Search implementation for low-mass binaries
• The use of new coordinates for the template space in hierarchical search for gravitational waves from inspiraling binaries
• Spin-induced deformations and tests of binary black hole nature using third-generation detectors
• The General Relativistic Two Body Problem and the Effective One Body Formalism
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• Archival searches for stellar-mass binary black holes in LISA
• Interpreting the results of searches for gravitational waves from coalescing binaries
• Generic bounds on dipolar gravitational radiation from inspiralling compact binaries
• Mathisson-Papapetrou-Tulczyjew-Dixon (MPTD) equations in ultra-relativistic regime and gravimagnetic moment
• Tidal Stablization of Neutron Stars and White Dwarfs
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: From Source to Canonical Moment
• Three Dimensional Distorted Black Holes
• Proposal for Determining the Total Masses of Eccentric Binaries Using Signature of Periastron Advance in Gravitational Waves
• Intermediate-mass-ratio-inspirals in the Einstein Telescope: I. Signal-to-noise ratio calculations
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: II. Dimensional Regularization and Renormalization
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Tests of General Relativity and Alternative theories of gravity using Gravitational Wave observations
• Gravitational Wave Emission From a Binary Black Hole System in Presence of an Accretion Disk
• Particle Swarm Optimization and gravitational wave data analysis: Performance on a binary inspiral testbed
• Gravitational Interaction of Spinning Bodies, Center-of-Mass Coordinate and Radiation of Compact Binary Systems
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Sub-threshold binary neutron star search in Advanced LIGO's first observing run
• Multivariate Classification with Random Forests for Gravitational Wave Searches of Black Hole Binary Coalescence
• Gravitational Waves from the Inspiral of Supermassive Black Holes in Galactic-scale Simulations
• Importance of including small body spin effects in the modelling of intermediate mass-ratio inspirals. II Accurate parameter extraction of strong sources using higher-order spin effects
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• Advanced localization of massive black hole coalescences with LISA
• Parameter estimation of coalescing supermassive black hole binaries with LISA
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: Relating the Harmonic and Radiative Metrics
• Effects of finite arm-length of LISA on analysis of gravitational waves from MBH binaries
• Computing the Complete Gravitational Wavetrain from Relativistic Binary Inspiral
• Comparing the inspiral of irrotational and corotational binary neutron stars
• The central density of neutron stars in close binaries
• Ineffectiveness of Padé resummation techniques in post-Newtonian approximations
• Detectability of lensed gravitational waves in matched-filtering searches
• Fast Parameter Estimation of Binary Mergers for Multimessenger Followup
• Symmetries of post-Galilean expansions
• Analyzing Gravitational Waves with General Relativity
• Theory of post-Newtonian radiation and reaction
• Head-on collision of compact objects in general relativity: Comparison of post-Newtonian and perturbation approaches
• Testing GR with the Gravitational Wave Inspiral Signal GW170817
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• About gravitational-wave generation by a three-body system
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Parameter estimation of compact binaries using the inspiral and ringdown waveforms
• Particle Swarm Optimization based search for gravitational waves from compact binary coalescences: performance improvements
• Solving the Darwin problem in the first post-Newtonian approximation of general relativity
• Coincidence analysis to search for inspiraling compact binaries using TAMA300 and LISM data
• Rapid pre-merger localization of binary neutron stars in third generation gravitational wave detectors
• A faster implementation of the hierarchical search algorithm for detection of gravitational waves from inspiraling compact binaries
• Binaries Wandering Around Supermassive Black Holes Due To Gravito-electromagnetism
• Establishing significance of gravitational-wave signals from a single observatory in the PyCBC offline search
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• Radiation Reaction for Non-Spinning Bodies at 4.5PN in the Effective Field Theory Approach
• Deep Learning Model on Gravitational Waveforms in Merging and Ringdown Phases of Binary Black Hole Coalescences
• Performance of Particle Swarm Optimization on the fully-coherent all-sky search for gravitational waves from compact binary coalescences
• A blind hierarchical coherent search for gravitational-wave signals from coalescing compact binaries in a network of interferometric detectors
• Probing evolution of binaries influenced by the spin-orbit resonances
• Extracting the three- and four-graviton vertices from binary pulsars and coalescing binaries
• Computational Resources to Filter Gravitational Wave Data with P-approximant Templates
• Rates of Short-GRB afterglows in association with Binary Neutron Star mergers
• Towards a real-time fully-coherent all-sky search for gravitational waves from compact binary coalescences using particle swarm optimization
• $f$-mode Imprints in Gravitational Waves from Coalescing Binaries involving Aligned Spinning Neutron Stars
• Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
• Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
• The Post Minkowskii Expansion of General Relativity
• New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test-mass in the Schwarzschild spacetime
• Tensor-Multi-Scalar Gravity: Equations of Motion to 2.5 post-Newtonian Order
• Gravitational waves from coalescing binaries and Doppler experiments
• Prompt sky localization of compact binary sources using a meshfree approximation
• Toward the search for gravitational waves from inspiralling compact binaries in TAMA300 data during 2003: data quality and stability
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Parameter estimation of neutron star-black hole binaries using an advanced gravitational-wave detector network: Effects of the full post-Newtonian waveform
• Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• Parametrized tests of general relativity using eccentric compact binaries
• Gravitational Wavetrains in the Quasi-Equilibrium Approximation: A Model Problem in Scalar Gravitation
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Premerger phenomena in neutron-star binary coalescences
• Exploring Short-GRB afterglow parameter space for observations in coincidence with gravitational waves
• Detectability of gravitational higher order modes in the third-generation era
• Gravitational waves from binary systems in circular orbits: Does the post-Newtonian expansion converge?
• Improved gravitational waveforms from spinning black hole binaries
• Testing pseudo-complex general relativity with gravitational waves
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• Radiating Love: adiabatic tidal fluxes and modes up to next-to-next-to-leading post-Newtonian order
• Detection Confidence Tests for Burst and Inspiral Candidate Events
• Astronomy and astrophysics with gravitational waves in the Advanced Detector Era
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Schwarzschild Fuzzball and Explicitly Unitary Hawking Radiations
• Parameter Estimation with Nonstationary Noise in Gravitational-wave Data
• Approximate Black Holes for Numerical Relativity
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• On the point mass approximation to calculate the gravitational wave signal from white dwarf binaries
• Obtaining Gravitational Waves from Inspiral Binary Systems using LIGO data
• Gravitational wave extraction in higher dimensional numerical relativity using the Weyl tensor
• Gravitational Wave Chirp Search: Economization of PN Matched Filter Bank via Cardinal Interpolation
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• An $\dot{f}(f)$-frequency dynamics algorithm for gravitational waves
• Impact of gravitational waveform model systematics on the measurement of the Hubble constant
• Mother templates for gravitational wave chirps
• A New Template Family For The Detection Of Gravitational Waves From Comparable Mass Black Hole Binaries
• Gravitational radiation from corotating binary neutron stars of incompressible fluid in the first post-Newtonian approximation of general relativity
• Gravitational waves from inspiraling binary black holes
• Tanaka-Tagoshi Parametrization of post-1PN Spin-Free Gravitational Wave Chirps: Equispaced and Cardinal Interpolated Lattices For First Generation Interferometric Antennas
• Analytic Approximations in GR and Gravitational Waves
• The gravitational wave symphony of the Universe
• Gravitational-wave searches in the era of Advanced LIGO and Virgo
• Coincidence analysis to search for inspiraling compact binaries
• Recent LIGO-Virgo discoveries
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Fast and faithful interpolation of numerical relativity surrogate waveforms using meshfree approximation
• Renormalized 2PN spin contributions to the accumulated orbital phase for LISA sources
• Gravitational-wave signatures of mirror (a)symmetry in binary black hole mergers: measurability and correlation to gravitational-wave recoil
• Black Hole and Neutron Star Binaries: Theoretical Challenges
• Gravitational radiation sources and signatures
• On the role of magnetic fields into the dynamics and gravitational wave emission of binary neutron stars
• Searches for Gravitational Waves from Binary Neutron Stars: A Review
• LIGO's "Science Reach"
• Complete adiabatic waveform templates for a test-mass in the Schwarzschild spacetime: VIRGO and Advanced LIGO studies
• Tests of general relativity at the fourth post-Newtonian order
• The Statistical Mechanics of Horizons and Black Hole Thermodynamics
• Modelling the post-Newtonian test-mass gravitational wave flux function for compact binary systems using Chebyshev polynomials
• The Cauchy convergence of T and P-approximant templates for test-mass Kerr binary systems
• Matched filters for coalescing binaries detection on massively parallel computers
• Microscopic State of BHs and an Exact One Body Method for Binary Dynamics in General Relativity
• Can the Near-Horizon Black Hole Memory be detected through Binary Inspirals?
• More on Tanaka-Tagoshi Parametrization of post-1PN Spin-Free Gravitational Wave Chirps: Equispaced and Cardinal Interpolated Lattices
• A Parametrized Test of General Relativity for LISA Massive Black Hole Binary Inspirals
• Space-time Schrödinger symmetries of a post-Galilean particle
• Glitch veto based on unphysical gravitational wave binary inspiral templates
• Introduction to the Analysis of Low-Frequency Gravitational Wave Data
• The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries
• The impact of relativistic corrections on the detectability of dark-matter spikes with gravitational waves
• Gravitational waves from binary systems in circular orbits: Convergence of a dressed multipole truncation
• Frequency domain analysis of the gravitational wave energy loss in hyperbolic encounters
• Equations of motion for compact binary systems in general relativity: Do they depend on the bodies' internal structure at the third post-Newtonian order?
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Gravitational physics in the context of Indian astronomy: A vision document
• Search for gravitational waves from binary black hole inspiral, merger and ringdown
• Detecting gravitational waves from test-mass bodies orbiting a Kerr black hole with P-approximant templates
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Searching for gravitational waves emitted by binaries with spinning components
• Degravitation and the relaxed Einstein equations
• 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
• Gravitational-wave constraints on noncommutative spacetime from GW190814
• Exact Results On the Number of Gravitons Radiated During Binary Inspiral