Effective one-body approach to general relativistic two-body dynamics

Abstract

We map the general relativistic two-body problem onto that of a test particle moving in an effective external metric. This effective-one-body approach defines, in a non-perturbative manner, the late dynamical evolution of a coalescing binary system of compact objects. The transition from the adiabatic inspiral, driven by gravitational radiation damping, to an unstable plunge, induced by strong spacetime curvature, is predicted to occur for orbits more tightly bound than the innermost stable circular orbit in a Schwarzschild metric of mass M = m1 + m2. The binding energy, angular momentum and orbital frequency of the innermost stable circular orbit for the time-symmetric two-body problem are determined as a function of the mass ratio.

52 pages, RevTex, epsfig, 8 figures

Cited by in corpus (908)

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• Conservative corrections to the innermost stable circular orbit (ISCO) of a Kerr black hole: a new gauge-invariant post-Newtonian ISCO condition, and the ISCO shift due to test-particle spin and the gravitational self-force
• Suitability of post-Newtonian/numerical-relativity hybrid waveforms for gravitational wave detectors
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence: Further investigations
• Analytic self-force calculations in the post-Newtonian regime: eccentric orbits on a Schwarzschild background
• Implications of the Gravitational Wave Event GW150914
• New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects
• Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM
• Spherical harmonic modes of 5.5 post-Newtonian gravitational wave polarizations and associated factorized resummed waveforms for a particle in circular orbit around a Schwarzschild black hol
• Search for Gravitational Waves from Intermediate Mass Binary Black Holes
• Introductory lectures on the Effective One Body formalism
• Comparing Gravitational Waveform Extrapolation to Cauchy-Characteristic Extraction in Binary Black Hole Simulations
• Gravitational wave emission from binary supermassive black holes
• Frequency-domain algorithm for the Lorenz-gauge gravitational self-force
• Confirming and improving post-Newtonian and effective-one-body results from self-force computations along eccentric orbits around a Schwarzschild black hole
• Impact of high-order tidal terms on binary neutron-star waveforms
• Multiband Observation of LIGO/Virgo Binary Black Hole Mergers in the Gravitational-wave Transient Catalog GWTC-1
• Waveform accuracy and systematic uncertainties in current gravitational wave observations
• Pseudospectrum and binary black hole merger transients
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Status of NINJA: the Numerical INJection Analysis project
• Analytical high-order post-Newtonian expansions for spinning extreme mass ratio binaries
• Status of black-hole-binary simulations for gravitational-wave detection
• Gravitational waves from merging compact binaries
• Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code
• Testing the multipole structure of compact binaries using gravitational wave observations
• Second-order perturbation theory: problems on large scales
• The SXS Collaboration's third catalog of binary black hole simulations
• Effective Field Theory for Extreme Mass Ratios
• Tests of general relativity in the nonlinear regime: a parametrized plunge-merger-ringdown gravitational waveform model
• Hamiltonian Formulation of the Conservative Self-Force Dynamics in the Kerr Geometry
• Extreme mass ratio inspirals on the equatorial plane in the adiabatic order
• On the Neutron Star-Black Hole Binaries Produced by Binary-driven-Hypernovae
• Reliability of complete gravitational waveform models for compact binary coalescences
• Gravitational-wave versus X-ray tests of strong-field gravity
• Ruling Out Chaos in Compact Binary Systems
• Improving gravitational-wave parameter estimation using Gaussian process regression
• Gravitational shock waves and scattering amplitudes
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• Tidal Interaction between a Fluid Star and a Kerr Black Hole in Circular Orbit
• Comparison of high-accuracy numerical simulations of black-hole binaries with stationary phase post-Newtonian template waveforms for Initial and Advanced LIGO
• Faithful effective-one-body waveform of small-mass-ratio coalescing black hole binaries: the eccentric, nonspinning, case
• On the motion of hairy black holes in Einstein-Maxwell-dilaton theories
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?
• Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case
• Radiation reaction at 3.5 post-Newtonian order in effective field theory
• A Precessing Numerical Relativity Waveform Surrogate Model for Binary Black Holes: A Gaussian Process Regression Approach
• Gravitational scattering at the seventh order in $G$: nonlocal contribution at the sixth post-Newtonian accuracy
• Comparison of post-Minkowskian and self-force expansions: Scattering in a scalar charge toy model
• Measuring precession in asymmetric compact binaries
• Length requirements for numerical-relativity waveforms
• Probing the equation of state of neutron star matter with gravitational waves from binary inspirals in light of GW170817: a brief review
• Spin-multipole effects in binary black holes and the test-body limit
• Gyroscopes orbiting black holes: A frequency-domain approach to precession and spin-curvature coupling for spinning bodies on generic Kerr orbits
• Inferring eccentricity evolution from observations of coalescing binary black holes
• Analytic determination of the eight-and-a-half post-Newtonian self-force contributions to the two-body gravitational interaction potential
• Measuring intermediate mass black hole binaries with advanced gravitational wave detectors
• Astrophysics of Super-massive Black Hole Mergers
• The Subleading Eikonal in Supergravity Theories
• Hamiltonians and canonical coordinates for spinning particles in curved space-time
• Dynamics of Black Hole Pairs II: Spherical Orbits and the Homoclinic Limit of Zoom-Whirliness
• Detection and Parameter Estimation of Gravitational Waves from Compact Binary Inspirals with Analytical Double-Precessing Templates
• Accuracy of binary black hole waveform models for aligned-spin binaries
• New Avenue for Accurate Analytical Waveforms and Fluxes for Eccentric Compact Binaries
• On the four-loop static contribution to the gravitational interaction potential of two point masses
• Relativistic orbits around spinning supermassive black holes. Secular evolution to 4.5 post-Newtonian order
• Tests of general relativity using multiband observations of intermediate mass binary black hole mergers
• Adding eccentricity to quasicircular binary-black-hole waveform models
• Black hole perturbation theory and multiple polylogarithms
• Modeling Equal and Unequal Mass Binary Neutron Star Mergers Using Public Codes
• Analytical Black-Hole Binary Merger Waveforms
• Scalar QED as a toy model for higher-order effects in classical gravitational scattering
• A Rosetta Stone for eccentric gravitational waveform models
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• EFTofPNG: A package for high precision computation with the Effective Field Theory of Post-Newtonian Gravity
• Strong-field scattering of two spinning black holes: Numerics versus Analytics
• Towards a gravitational self force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals
• Uncertainty in hybrid gravitational waveforms: Optimizing initial orbital frequencies for binary black-hole simulations
• Constraints on the binary black hole nature of GW151226 and GW170608 from the measurement of spin-induced quadrupole moments
• Spectral analysis of gravitational waves from binary neutron star merger remnants
• A surrogate model for gravitational waveforms of spin-aligned binary black holes with eccentricities
• A Review of Gravitational Memory and BMS Frame Fixing in Numerical Relativity
• A Fermi Gamma-ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-Wave Candidates in Advanced LIGO's First Observing Run
• New gravitational self-force analytical results for eccentric orbits around a Schwarzschild black hole
• Comparing Effective One Body Hamiltonians for spin-aligned coalescing binaries
• Analytic gravitational waveforms for generic precessing compact binaries
• Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
• Two-body problem in Scalar-Tensor theories as a deformation of General Relativity : an Effective-One-Body approach
• Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins
• Factorization and resummation: A new paradigm to improve gravitational wave amplitudes. II: the higher multipolar modes
• An efficient iterative method to reduce eccentricity in numerical-relativity simulations of compact binary inspiral
• Constraining the parameters of GW150914 & GW170104 with numerical relativity surrogates
• Lorenz gauge gravitational self-force calculations of eccentric binaries using a frequency domain procedure
• Horizon radiation reaction forces
• Can the post-Newtonian gravitational waveform of an inspiraling binary be improved by solving the energy balance equation numerically?
• Accelerating the evaluation of inspiral-merger-ringdown waveforms with adapted grids
• Phase shift of gravitational waves induced by aberration
• Complete phenomenological gravitational waveforms from spinning coalescing binaries
• Complete conservative dynamics for inspiralling compact binaries with spins at the fourth post-Newtonian order
• Using Deep Learning to Localize Gravitational Wave Sources
• Reducing the two-body problem in scalar-tensor theories to the motion of a test particle : a scalar-tensor effective-one-body approach
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Gravitational Spin-Orbit Hamiltonian at NNNLO in the post-Newtonian framework
• Accurate inspiral-merger-ringdown gravitational waveforms for non-spinning black-hole binaries including the effect of subdominant modes
• Impact of Numerical Relativity information on effective-one-body waveform models
• Eccentric-orbit EMRI gravitational wave energy fluxes to 7PN order
• Measuring neutron star tidal deformability with Advanced LIGO: a Bayesian analysis of neutron star - black hole binary observations
• Third post-Newtonian effective-one-body Hamiltonian in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity
• Spin-orbit precession along eccentric orbits for extreme mass ratio black hole binaries and its effective-one-body transcription
• Precession-tracking coordinates for simulations of compact-object-binaries
• Mode coupling of Schwarzschild perturbations: Ringdown frequencies
• Completing the Fifth PN Precision Frontier via the EFT of Spinning Gravitating Objects
• Linear-in-mass-ratio contribution to spin precession and tidal invariants in Schwarzschild spacetime at very high post-Newtonian order
• Horizon-absorbed energy flux in circularized, nonspinning black-hole binaries and its effective-one-body representation
• Detweiler's gauge-invariant redshift variable: analytic determination of the nine and nine-and-a-half post-Newtonian self-force contributions
• The Kepler equation for inspiralling compact binaries
• Gravitomagnetic tidal effects in gravitational waves from neutron star binaries
• Assessing the model waveform accuracy of gravitational waves
• Unveiling the merger structure of black hole binaries in generic planar orbits
• An effective action model of dynamically scalarizing binary neutron stars
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• Spin contributions to the gravitational-waveform modes for spin-aligned binaries at the 3.5PN order
• Prompt Mergers of Neutron Stars with Black Holes
• Calabi-Yau meets Gravity: A Calabi-Yau three-fold at fifth post-Minkowskian order
• Detecting the Beaming Effect of Gravitational Waves
• Searching for ringdown higher modes with a numerical relativity-informed post-merger model
• A conservative effect of the second-order gravitational self-force on quasicircular orbits in Schwarzschild spacetime
• Construction of initial data for 3+1 numerical relativity
• Radiative losses and radiation-reaction effects at the first post-Newtonian order in Einstein-Cartan theory
• News from horizons in binary black hole mergers
• The General Relativistic Two Body Problem and the Effective One Body Formalism
• N${}^3$LO Quadratic-in-Spin Interactions for Generic Compact Binaries
• Spin-dependent two-body interactions from gravitational self-force computations
• Effective-One-Body Numerical-Relativity waveform model for Eccentric spin-precessing binary black hole coalescence
• Prospects for Measuring the Hubble Constant with Neutron-Star-Black-Hole Mergers
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• New effective precession spin for modeling multimodal gravitational waveforms in the strong-field regime
• Numerical simulations of black-hole binaries and gravitational wave emission
• Bounds on spinning particles in their innermost stable circular orbits around rotating braneworld black hole
• Experimental mathematics meets gravitational self-force
• General Relativistic Dynamics of an Extreme Mass-Ratio Binary interacting with an External Body
• Simple procedures to reduce eccentricity of binary black hole simulations
• Interpreting the results of searches for gravitational waves from coalescing binaries
• Multi-waveform inference of gravitational waves
• General-relativistic treatment of tidal $g$-mode resonances in coalescing binaries of neutron stars. I. Theoretical framework and crust breaking
• New Kludge Scheme for the Construction of Approximate Waveforms for Extreme-Mass-Ratio Inspirals
• N${}^3$LO Spin-Orbit Interaction via the EFT of Spinning Gravitating Objects
• Gravitational waveforms for spinning compact binaries
• Modelling gravitational waves from precessing black-hole binaries: Progress, challenges and prospects
• Fast Radio Bursts From Primordial Black Hole Binaries Coalescence
• Quadratic-in-spin interactions at fifth post-Newtonian order probe new physics
• Probing the Black Hole Metric. I. Black Hole Shadows and Binary Black-Hole Inspirals
• Bethe-Salpeter equation for classical gravitational bound states
• Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals
• Numerical computation of the EOB potential q using self-force results
• Redshift factor and the first law of binary black hole mechanics in numerical simulations
• Intermediate-mass-ratio-inspirals in the Einstein Telescope: I. Signal-to-noise ratio calculations
• High post-Newtonian order gravitational self-force analytical results for eccentric orbits around a Kerr black hole
• Quasi-5.5PN TaylorF2 approximant for compact binaries: point-mass phasing and impact on the tidal polarizability inference
• Compact Binary Waveform Center-of-Mass Corrections
• Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
• Effective-one-body waveforms for extreme-mass-ratio binaries: Consistency with second-order gravitational self-force quasicircular results and extension to nonprecessing spins and eccentricity
• Boundary to bound dictionary for generic Kerr orbits
• A new effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
• First gravitational-wave search for intermediate-mass black hole mergers with higher order harmonics
• Inferring the gravitational wave memory for binary coalescence events
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• Gauge Invariant Perturbations of General Spherically Symmetric Spacetimes
• Post-Minkowskian Theory Meets the Spinning Effective-One-Body Approach for Two-Body Scattering
• Stability of nonspinning effective-one-body model in approximating two-body dynamics and gravitational-wave emission
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Towards beating the curse of dimensionality for gravitational waves using Reduced Basis
• Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN
• Quasi-equilibrium Binary Black Hole Initial Data for Dynamical Evolutions
• Light-ray operators, detectors and gravitational event shapes
• Renormalizing Love: tidal effects at the third post-Newtonian order
• On the detectability of higher harmonics with LISA
• Leveraging gravitational-wave memory to distinguish neutron star--black hole binaries from black hole binaries
• Assessing the Energetics of Spinning Binary Black Hole Systems
• Tidal interaction in compact binaries: a post-Newtonian affine framework
• ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
• Gravitational Waveforms for Precessing, Quasicircular Compact Binaries with Multiple Scale Analysis: Small Spin Expansion
• Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
• Binary neutron star merger simulations with different initial orbital frequency and equation of state
• Deviation of quadrupolar bodies from geodesic motion in a Kerr spacetime
• Analytic solutions for the motion of spinning particles near spherically symmetric black holes and exotic compact objects
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Fast spectral source integration in black hole perturbation calculations
• Numerical black hole initial data with low eccentricity based on post-Newtonian orbital parameters
• Upgraded waveform model of eccentric binary black hole based on effective-one-body-numerical-relativity for spin-aligned binary black holes
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• Binary black hole spacetimes with a helical Killing vector
• Exploring waveforms with non-GR deviations for extreme mass-ratio inspirals
• Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral
• Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• Numerical-relativity validation of effective-one-body waveforms in the intermediate-mass-ratio regime
• GRB 140619B: a short GRB from a binary neutron star merger leading to black hole formation
• Post-Newtonian Waveforms from Spinning Scattering Amplitudes
• Parameter estimation of coalescing supermassive black hole binaries with LISA
• Gravitational Bound Waveforms from Amplitudes
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Octupolar invariants for compact binaries on quasi-circular orbits
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• Testing regular black holes with X-ray and GW data
• Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
• Remodeling the Effective One-Body Formalism in Post-Minkowskian Gravity
• Gravitational waves from spinning binary black holes at the leading post-Newtonian orders at all orders in spin
• Self-force framework for transition-to-plunge waveforms
• Comparing Hamiltonians of a spinning test particle for different tetrad fields
• Gyroscope precession along bound equatorial plane orbits around a Kerr black hole
• Statistical and systematic uncertainties in extracting the source properties of neutron star - black hole binaries with gravitational waves
• New self-consistent effective one-body theory for spinless binaries based on the post-Minkowskian approximation
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
• Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods
• Resonant recoil in extreme mass ratio binary black hole mergers
• Gravitational-wave echoes from numerical-relativity waveforms via space-time construction near merging compact objects
• Generating exact solutions to Einstein's equation using linearized approximations
• Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling for two nonprecessing black holes with aligned spins
• Comparing the inspiral of irrotational and corotational binary neutron stars
• Astrophysical Implications of Neutron Star Inspiral and Coalescence
• Self-consistent Effective-one-body theory for spinless binaries based on post-Minkowskian approximation I: Hamiltonian and decoupled equation for ${\psi }_4^B$
• Including mode mixing in a higher-multipole model for gravitational waveforms from nonspinning black-hole binaries
• Conservative second-order gravitational self-force on circular orbits and the effective one-body formalism
• Relativistic mergers of compact binaries in clusters: The fingerprint of the spin
• Population inference of spin-induced quadrupole moments as a probe for non-black hole compact binaries
• Searching for near-horizon quantum structures in the binary black-hole stochastic gravitational-wave background
• Gravitational-wave inference for eccentric binaries: the argument of periapsis
• Deep Generative Models of Gravitational Waveforms via Conditional Autoencoder
• Binary mergers in strong gravity background of Kerr black hole
• Self-force effects on the marginally bound zoom-whirl orbit in Schwarzschild spacetime
• Self-consistent effective-one-body theory for spinning binaries based on post-Minkowskian approximation
• Theory of post-Newtonian radiation and reaction
• Analyzing Gravitational Waves with General Relativity
• A sparse representation of gravitational waves from precessing compact binaries
• Ineffectiveness of Padé resummation techniques in post-Newtonian approximations
• Spin-orbit precession along eccentric orbits: improving the knowledge of self-force corrections and of their effective-one-body counterparts
• Observables from classical black hole scattering in Scalar-Tensor theory of gravity from worldline quantum field theory
• Symmetries of post-Galilean expansions
• GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications
• The physics of black hole binaries: geodesics, relaxation modes and energy extraction
• Template Banks for Binary black hole searches with Numerical Relativity waveforms
• Binary Dynamics from Worldline QFT for Scalar-QED
• Testing GR with the Gravitational Wave Inspiral Signal GW170817
• Gravitational self-force corrections to gyroscope precession along circular orbits in the Kerr spacetime
• The Close-Limit Approximation for Black Hole Binaries with Post-Newtonian Initial Conditions
• Photon surfaces with equipotential time-slices
• High-accuracy waveforms for black hole-neutron star systems with spinning black holes
• Gravitoelectric dynamical tides at second post-Newtonian order
• Radiation-balanced simulations for binary inspiral
• The gravitational capture of compact objects by massive black holes
• High-accuracy simulations of highly spinning binary neutron star systems
• Binary black hole detection rates in inspiral gravitational wave searches
• Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals from Black-hole Perturbation Approach
• Hybrid method for understanding black-hole mergers: Inspiralling case
• Classifying post-Minkowskian geometries for gravitational waves via loop-by-loop Baikov
• Detection and characterization of spin-orbit resonances in the advanced gravitational wave detectors era
• Method to estimate ISCO and ring-down frequencies in binary systems and consequences for gravitational wave data analysis
• Massive twistor worldline in electromagnetic fields
• Efficient Gravitational Wave Template Bank Generation with Differentiable Waveforms
• From the EFT of Spinning Gravitating Objects to Poincaré and Gauge Invariance at the 4.5PN Precision Frontier
• Understanding binary neutron star collisions with hypermodels
• Extreme mass ratio inspirals: perspectives for their detection
• Unbound motion on a Schwarzschild background: Practical approaches to frequency domain computations
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Dynamical tides during the inspiral of rapidly spinning neutron stars: Solutions beyond mode resonance
• Effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• New self-force method via elliptic partial differential equations for Kerr inspiral models
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Stringent Pulsar Timing Bounds on Light Scalar Couplings to Matter
• Analytical effective-one-body formalism for extreme-mass-ratio inspirals: eccentric orbits
• Endpoint of the up-down instability in precessing binary black holes
• A nonlinear scalar model of extreme mass ratio inspirals in effective field theory I. Self force through third order
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• Nonlocal-in-time effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Phenomenology and origin of late-time tails in eccentric binary black hole mergers
• Highly eccentric EMRI waveforms via fast self-forced inspirals
• Tidal deformability and gravitational-wave phase evolution of magnetised compact-star binaries
• Spinning compact binary dynamics and chameleon orbits
• High-Precision Ringdown Surrogate Model for Non-Precessing Binary Black Holes
• Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
• Post-Minkowskian Hamiltonians in Modified Theories of Gravity
• Gravitational Dyonic Amplitude at One-Loop and its Inconsistency with the Classical Impulse
• Radiative Classical Gravitational Observables at $\mathcal{O}(G^3)$ from Scattering Amplitudes
• 2.5PN accurate waveform information for generic-planar-orbit binaries in effective one-body models
• Scattering Amplitudes and N-Body Post-Minkowskian Hamiltonians in General Relativity and Beyond
• Advances in Simulations of Generic Black-Hole Binaries
• Degeneracy of gravitational waveforms in the context of GW150914
• $f$-mode Imprints in Gravitational Waves from Coalescing Binaries involving Aligned Spinning Neutron Stars
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Multi-scale Constraints on Scalar-Field couplings to Matter: The Geodetic and Frame-Dragging Effects
• The two-body potential of Vainshtein screened theories
• New gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole: redshift invariant
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• The H-graph with equal masses in terms of multiple polylogarithms
• New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test-mass in the Schwarzschild spacetime
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• Off-equatorial stable circular orbits for spinning particles
• A burst search for gravitational waves from binary black holes
• A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
• Testing gravity with Extreme-Mass-Ratio Inspirals
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Learning orbital dynamics of binary black hole systems from gravitational wave measurements
• Spin and Quadrupole Couplings for High Spin Equatorial Intermediate Mass-ratio Coalescences
• Efficient Estimation of Highly Structured Posteriors of Gravitational-Wave Signals with Markov-Chain Monte Carlo
• Excitation of high frequency voices from intermediate-mass-ratio inspirals with large eccentricity
• Initial data for black hole-neutron star binaries, with rotating stars
• Dynamical quasinormal mode excitation
• Late-time tails in nonlinear evolutions of merging black holes
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
• Evolution of inspiralling neutron star binaries: effects of tidal interactions and orbital eccentricities
• Geometrized effective-one-body formalism for extreme-mass-ratio limits: Generic orbits
• Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models
• Energy-conserving integrator for conservative Hamiltonian systems with ten-dimensional phase space
• Detecting transient gravitational waves in non-Gaussian noise with partially redundant analysis methods
• Influence of mass-ratio corrections in extreme-mass-ratio inspirals for testing general relativity
• Relativistic non-instantaneous action-at-a-distance interactions
• Multipolar gravitational waveforms and ringdowns generated during the plunge from the innermost stable circular orbit into a Schwarzschild black hole
• Reduction of the two-body dynamics to a one-body description in classical electrodynamics
• Radiation eikonal for post-Minkowskian observables
• Towards a unitary, renormalizable and ultraviolet-complete quantum theory of gravity
• New gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole: gyroscope precession
• Using gravitational waves to distinguish between neutron stars and black holes in compact binary mergers
• Detweiler's redshift invariant for spinning particles along circular orbits on a Schwarzschild background
• Post-Newtonian expansions of extreme mass ratio inspirals of spinning bodies into Schwarzschild black holes
• Strong Field Scattering of Black Holes: Assessing Resummation Strategies
• Gravitational Waves versus X and Gamma Ray Emission in a Short Gamma-Ray Burst
• Circular equatorial orbits of extended bodies with spin-induced quadrupole around a Kerr black hole: Comparing spin-supplementary conditions
• Effective one-body approach to the relativistic two-body problem
• Initial Conditions for Numerical Relativity -- Introduction to numerical methods for solving elliptic PDEs
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• Actions of spinning compact binaries: Spinning particle in Kerr matched to dynamics at 1.5 post-Newtonian order
• Detectability of gravitational higher order modes in the third-generation era
• Improving performance of SEOBNRv3 by $\sim$300x
• Charged test-particle scattering and effective one-body metrics with spin
• The 2.5PN linear momentum flux and associated recoil from inspiralling compact binaries in quasi-circular orbits: Nonspinning case
• Black-Hole Neutron Star Simulations with the BAM code: First Tests and Simulations
• Premerger phenomena in neutron-star binary coalescences
• Searching for binary coalescences with inspiral templates: Detection and parameter estimation
• Fast Evolution and Waveform Generator for Extreme-Mass-Ratio Inspirals in Equatorial-Circular Orbits
• A template bank to search for gravitational waves from inspiralling compact binaries: II. Phenomenological model
• Detweiler's redshift invariant for extended bodies orbiting a Schwarzschild black hole
• Comment on "Gravity Waves, Chaos, and Spinning Compact Binaries"
• Conservative Scattering of Reissner-Nordström Black Holes at Third Post-Minkowskian Order
• Systematic errors in measuring parameters of non-spinning compact binary coalescences with post-Newtonian templates
• Improved gravitational waveforms from spinning black hole binaries
• Merger states and final states of black hole coalescences: a numerical-relativity-assisted effective-one-body approach
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• An effective-gravity perspective on the Sun-Jupiter-comet three-body system
• Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT
• Real modes and null memory contributions in effective-one-body models
• Exact Gravitational Wave Signatures from Colliding Extreme Black Holes
• Beyond general relativity: designing a template-based search for exotic gravitational wave signals
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
• High-accuracy high-mass ratio simulations for binary neutron stars and their comparison to existing waveform models
• Source localizations with the network of space-based gravitational wave detectors
• Gravitational spin-orbit dynamics at the fifth-and-a-half post-Newtonian order
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Schwarzschild Fuzzball and Explicitly Unitary Hawking Radiations
• Bound States of the Schwarzschild Black Hole
• Peaking into the abyss: Characterizing the merger of equatorial-eccentric-geodesic plunges in rotating black holes
• Comparing Criteria for Circular Orbits in General Relativity
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• GPU-accelerated LISA parameter estimation with full time domain response
• Novel Screening with Two Bodies: Summing the ladder in disformal scalar-tensor theories
• Efficient simulations of high-spin black holes with a new gauge
• Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Gravitational self-force corrections to tidal invariants for particles on eccentric orbits in a Schwarzschild spacetime
• Action-angle variables of a binary black hole with arbitrary eccentricity, spins, and masses at 1.5 post-Newtonian order
• Gravitational self-force corrections to tidal invariants for spinning particles on circular orbits in a Schwarzschild spacetime
• Effective metric of spinless binaries with radiation-reaction effect up to fourth Post-Minkowskian order in effective-one-body theory
• Waveforms from Amplitudes
• High-energy hyperbolic scattering by neutron stars and black holes
• The Design Strain Sensitivity of the Schenberg Spherical Resonant Antenna for Gravitational Waves
• More about scalar gravity
• Gravitational Wave Chirp Search: Economization of PN Matched Filter Bank via Cardinal Interpolation
• Gravitational waves in massive gravity: Waveforms generated by a particle plunging into a black hole and the excitation of quasinormal modes and quasibound states
• Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
• Half-solution to the two-body problem in General Relativity
• Classification of Feynman integral geometries for black-hole scattering at 5PM order
• Highly accurate simulations of asymmetric black-hole scattering and cross validation of effective-one-body models
• Binary black holes in Mkns as sources of gravitational radiation for space based interferometers
• High-Accuracy Comparison between the Post-Newtonian and Self-Force Dynamics of Black-Hole Binaries
• Gravitational waveforms for finite mass binaries
• Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
• Spinning waveforms of scalar radiation in quadratic modified gravity
• Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order
• A Post-Newtonian approach to black hole-fluid systems
• Analytical determination of the periastron advance in spinning binaries from self-force computations
• Enhancing gravitational waveform models through dynamic calibration
• Self-forced evolutions of an implicit rotating source: A natural framework to model comparable and intermediate mass-ratio systems from inspiral through ringdown
• Gravitational self-force corrections to tidal invariants for particles on circular orbits in a Kerr spacetime
• Energy and angular momentum radiated for non head-on binary black hole collisions
• Waveforms produced by a scalar point particle plunging into a Schwarzschild black hole: Excitation of quasinormal modes and quasibound states
• A New Template Family For The Detection Of Gravitational Waves From Comparable Mass Black Hole Binaries
• Testing the Boundary-to-Bound Correspondence with Numerical Relativity
• Nonradial oscillations of stratified neutron stars with solid crusts: Mode characterization and tidal resonances in coalescing binaries
• Analytic Approximations in GR and Gravitational Waves
• Energy flux and waveforms by coalescing spinless binary system in effective one-body theory
• Binary Black Hole Coalescence in Semi-Analytic Puncture Evolution
• Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
• Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results
• Testing gravitational waveform models using angular momentum
• Astrophysics with the Laser Interferometer Space Antenna
• Tanaka-Tagoshi Parametrization of post-1PN Spin-Free Gravitational Wave Chirps: Equispaced and Cardinal Interpolated Lattices For First Generation Interferometric Antennas
• Gravitational waves from inspiraling binary black holes
• Characterizing the effect of eccentricity on the dynamics of binary black hole mergers in numerical relativity
• Padé approximants for truncated post-Newtonian neutron star models
• Black holes in General Relativity and beyond
• Numerical relativity simulations in the era of the Einstein Telescope
• Resonant Islands of Effective-One-Body Dynamics
• Gravitational and electromagnetic emission by magnetized coalescing binary systems
• Gravitational waves from quasielliptic compact binaries in scalar-tensor theory to one-and-a-half post-Newtonian order
• The first law of binary black hole scattering
• Success of the small mass ratio approximation during the final orbits of binary black hole simulations
• Scattering of uncharged particles in the field of two extremely charged black holes
• Solar system dynamics in general relativity
• Some new perspectives on the Kruskal--Szekeres extension with applications to photon surfaces
• Massive to gauge field reduction and gravitational wave zone information
• Arrival Times of Gravitational Radiation Peaks for Binary Inspiral
• On the foundations of general relativistic celestial mechanics
• The general relativistic two body problem
• Testing the validity of the phenomenological gravitational waveform models for nonspinning binary black hole searches at low masses
• Testing dispersion of gravitational waves from eccentric extreme-mass-ratio inspirals
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Correlator Bank Detection of GW chirps. False-Alarm Probability, Template Density and Thresholds: Behind and Beyond the Minimal-Match Issue
• Observable Signatures of EMRI Black Hole Binaries Embedded in Thin Accretion Disks
• The Effective One Body description of the Two-Body problem
• Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
• Optimizing Neural Network Surrogate Models: Application to Black Hole Merger Remnants
• Probing Particle Physics with Gravitational Waves
• Probing the formation of the seeds of supermassive black holes with gravitational waves
• Gravitational-wave searches in the era of Advanced LIGO and Virgo
• On ab initio-based, free and closed-form expressions for gravitational waves
• Scrambling and Entangling Spinning Particles
• Black-Hole Perturbation Plus Post-Newtonian Theory: Hybrid Waveform for Neutron Star Binaries
• A complete waveform comparison of post-Newtonian and numerical relativity in eccentric orbits
• Relativistic encounters in dense stellar systems
• Trumpet Initial Data for Boosted Black Holes
• Testing merging of Dark Exotic Stars from Gravitational Waves in the Multi-messenger approach
• Advancing the Effective-One-Body Framework in the Test-Mass Limit
• Classical gravitational scattering from a gauge-invariant double copy
• General Relativistic Dynamics of Compact Binary Systems
• An Effective Field Theory for Binary Cosmic Strings
• The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• Unveiling the electrodynamic nature of spacetime collisions
• Report on the first binary black hole inspiral search in LIGO data
• Comparison of neural network architectures for feature extraction from binary black hole merger waveforms
• Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
• Probing Fundamental Physics with Gravitational Waves
• Dynamics for Super-Extremal Kerr Binary Systems at $\mathcal{O}(G^2)$
• Black Hole and Neutron Star Binaries: Theoretical Challenges
• Pseudo-topological Quasi-local Energy of Torsion Gravity
• Gravitational waveform model based on photon motion for spinning black holes
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Eccentric Pairs: Analytic Gravitational Waves from Binary Black Holes in Elliptic Orbits
• Gravitational scattering of two neutron stars
• Strong Field Scattering of Two Black Holes: Exploring Gauge Flexibility
• Gravitational waves from binary axionic black holes
• A public framework for Feynman calculations and post-Newtonian gravity
• Repeated Bursts: Gravitational Waves from Highly Eccentric Binaries
• Gravitational cubic-in-spin interaction at the next-to-leading post-Newtonian order
• Microscopic State of BHs and an Exact One Body Method for Binary Dynamics in General Relativity
• Last orbits of binary black holes
• Asymptotically matched quasi-circular inspiral and transition-to-plunge in the small mass ratio expansion
• Two-body problem in curved spacetime: exploring gravitational wave transient cases
• Constants of motion in gravitational self-force theory
• Orbital effects due to gravitational induction
• Calibrating approximate Bayesian credible intervals of gravitational-wave parameters
• Testing black hole metrics with binary black hole inspirals
• The Eikonal Approximation and the Gravitational Dynamics of Binary Systems
• Gravitational-wave signatures of nonviolent nonlocality
• Modelling the post-Newtonian test-mass gravitational wave flux function for compact binary systems using Chebyshev polynomials
• Dimer problem on a spherical surface
• Connecting Numerical Relativity and Data Analysis of Gravitational Wave Detectors
• Analysis of late-time tails in spin-aligned eccentric binary black hole mergers
• Three models of non-perturbative quantum-gravitational binding
• High-order effective-one-body tidal interactions and gravitational scattering
• Scattering Amplitudes for Binary Systems beyond GR
• Gravitational radiation reaction for compact binary systems at the fourth-and-a-half post-Newtonian order in harmonic coordinates
• Post-Newtonian Dynamics of Radiating Charges: Canonical Formulation and Binary Inspiral Laws
• Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation
• First-post-Newtonian generation of gravitational waves in Einstein-Cartan theory
• Compact binary system dynamics at the second post-Newtonian order: analytical formula of the coordinate time for eccentric and circular orbits
• GW250114 reveals black hole horizon signatures
• General Fourier expansion of post-Newtonian binary dynamics based on a quasi-Keplerian framework
• Tidal deformations of compact objects and gravitational wave emission
• Field theory for gravity at all scales
• Modeling Relative Peak Times of Gravitational Wave Harmonics
• Relativistic excitation of compact stars
• Extremely High-Order Convergence in Simulations of Relativistic Stars
• Radial infall of two compact objects: 2.5PN linear momentum flux and associated recoil
• Conditional Autoencoder for Generating Binary Neutron Star Waveforms with Tidal and Precession Effects
• Space-time Schrödinger symmetries of a post-Galilean particle
• Exploring gravitational impulse via quantum Boltzmann equation
• Bayesian analysis of analog gravity systems with the Rezzolla-Zhidenko metric
• Lagrange point stability for a rotating host mass binary
• A Mass-Shell Model of Compact Binary Coalescence
• The Radial Action from Probe Amplitudes to All Orders
• MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
• gr-Orbit-Toolkit: A Python-Based Software for Simulating and Visualizing Relativistic Orbits
• AthenaK simulations of the binary black hole merger GW150914
• Search for gravitational waves from binary black hole inspiral, merger and ringdown
• Fast Waveform Generation for Gravitational Waves using Evolutionary Algorithms
• Deep Residual Error and Bag-of-Tricks Learning for Gravitational Wave Surrogate Modeling
• Waveforms and fluxes: Towards a self-consistent effective one body waveform model for nonprecessing, coalescing black-hole binaries for third generation detectors
• Effective-one-body formalism for leading-order radiative effects in the post-linear framework
• The physics of gravitational waves
• Comparing eccentric waveform models based on post-Newtonian and effective-one-body approaches, over an observationally relevant parameter space
• Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
• Rising Tides: Analytic Modeling of Tidal Effects in Binary Neutron Star Mergers
• Constraining the Konoplya-Rezzolla-Zhidenko deformation parameters III: limits from stellar-mass black holes using gravitational-wave observations
• The influence of the mean anomaly on the dynamical quantities of binary black hole mergers in eccentric orbits
• Energetics and scattering of gravitational two-body systems at fourth post-Minkowskian order
• Hybrid waveforms for precessing quasi-circular binary systems
• Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves
• Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries
• Analytical solutions of bound timelike geodesic orbits in effective-one-body frame
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Relative motion in spacetime
• Assessment of Effective-One-Body Radiation Reactions for Generic Planar Orbits
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Precisely computing bound orbits of spinning bodies around black holes I: General framework and results for nearly equatorial orbits
• General Relativity from Quantum Field Theory
• Black hole sensitivities in Einstein-scalar-Gauss-Bonnet gravity
• Learning Post-Newtonian Corrections from Numerical Relativity
• Isotropic Coordinates for Generalized Schwarzschild-like Solutions
• Hamiltonian normal forms for the post-Newtonian binary problem