Transition from inspiral to plunge in binary black hole coalescences

Abstract

Combining recent techniques giving non-perturbative re-summed estimates of the damping and conservative parts of the two-body dynamics, we describe the transition between the adiabatic phase and the plunge, in coalescing binary black holes with comparable masses moving on quasi-circular orbits. We give initial dynamical data for numerical relativity investigations, with a fraction of an orbit left, and provide, for data analysis purposes, an estimate of the gravitational wave-form emitted throughout the inspiral, plunge and coalescence phases.

52 pages, 21 figures, ReVTex, epsfig; few misprints corrected

References in corpus (4)

• The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole
• Dynamical invariants for general relativistic two-body systems at the third post-Newtonian approximation
• Frequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binaries
• The close limit of colliding black holes: an update

Cited by in corpus (606)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• 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
• 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
• Quasinormal modes of black holes and black branes
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• Tests of general relativity with GW150914
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
• Properties of the Binary Black Hole Merger GW150914
• Physics, Astrophysics and Cosmology with Gravitational Waves
• Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
• Black holes, gravitational waves and fundamental physics: a roadmap
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
• 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
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Binary neutron-star mergers: a review of Einstein's richest laboratory
• Scattering Amplitudes and the Conservative Hamiltonian for Binary Systems at Third Post-Minkowskian Order
• GW150914: First results from the search for binary black hole coalescence with Advanced LIGO
• Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
• Inspiral, merger and ring-down of equal-mass black-hole binaries
• On the determination of the last stable orbit for circular general relativistic binaries at the third post-Newtonian approximation
• Effective-one-body model for black-hole binaries with generic mass ratios and spins
• Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals
• Amplitudes, Observables, and Classical Scattering
• Black Hole Binary Dynamics from the Double Copy and Effective Theory
• The SXS Collaboration catalog of binary black hole simulations
• A template bank for gravitational waveforms from coalescing binary black holes: non-spinning binaries
• Inspiral, merger and ringdown of unequal mass black hole binaries: a multipolar analysis
• Self-force and radiation reaction in general relativity
• Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
• Prospects for Fundamental Physics with LISA
• High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions
• Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
• Higher-order spin effects in the amplitude and phase of gravitational waveforms emitted by inspiraling compact binaries: Ready-to-use gravitational waveforms
• Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory
• Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach
• Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
• Gravitational self force in extreme mass-ratio inspirals
• High-energy gravitational scattering and the general relativistic two-body problem
• New Horizons for Fundamental Physics with LISA
• Dimensional regularization of the gravitational interaction of point masses
• Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects
• Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors
• Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
• A Comparison of search templates for gravitational waves from binary inspiral
• PyCBC Inference: A Python-based parameter estimation toolkit for compact binary coalescence signals
• Effective One Body description of tidal effects in inspiralling compact binaries
• Toward faithful templates for non-spinning binary black holes using the effective-one-body approach
• Transition from inspiral to plunge in precessing binaries of spinning black holes
• "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole
• Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit
• Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries
• Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian
• Modeling the complete gravitational wave spectrum of neutron star mergers
• Gravitational-Wave Inspiral of Compact Binary Systems to 7/2 Post-Newtonian Order
• Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
• Selection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence
• Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism
• Effective Field Theories of Post-Newtonian Gravity: A comprehensive review
• Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
• Black-hole binaries, gravitational waves, and numerical relativity
• Scattering Amplitudes and Conservative Binary Dynamics at $\mathcal{O}(G^4)$
• Modeling the dynamics of tidally-interacting binary neutron stars up to merger
• Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries
• Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-spinning, equal-mass black holes
• Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
• An improved analytical description of inspiralling and coalescing black-hole binaries
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• Observables and amplitudes for spinning particles and black holes
• Spinning Black Hole Binary Dynamics, Scattering Amplitudes and Effective Field Theory
• Scattering of two spinning black holes in post-Minkowskian gravity, to all orders in spin, and effective-one-body mappings
• Binary black hole merger dynamics and waveforms
• Numerical Relativity: A review
• An improved effective-one-body Hamiltonian for spinning black-hole binaries
• Estimating the final spin of a binary black hole coalescence
• Classical and quantum scattering in post-Minkowskian gravity
• Gravitational Self Force in a Schwarzschild Background and the Effective One Body Formalism
• Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
• Scattering Amplitudes, the Tail Effect, and Conservative Binary Dynamics at $O(G^4)$
• Frequency domain reduced order models for gravitational waves from aligned-spin compact binaries
• Analysis of LIGO data for gravitational waves from binary neutron stars
• The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole
• Including higher order multipoles in gravitational-wave models for precessing binary black holes
• Fourth post-Newtonian effective one-body dynamics
• A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries
• Phasing of gravitational waves from inspiralling eccentric binaries
• Gravitational self-force on a particle in eccentric orbit around a Schwarzschild black hole
• Radiative contribution to classical gravitational scattering at the third order in $G$
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with generic mass-ratios and spins
• Tidal effects in binary neutron star coalescence
• Comparing Effective-One-Body gravitational waveforms to accurate numerical data
• Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description
• Improved effective-one-body description of coalescing nonspinning black-hole binaries and its numerical-relativity completion
• Untangling the merger history of massive black holes with LISA
• A data-analysis driven comparison of analytic and numerical coalescing binary waveforms: nonspinning case
• The effect of gravitational-wave recoil on the demography of massive black holes
• Holomorphic Classical Limit for Spin Effects in Gravitational and Electromagnetic Scattering
• A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries
• Accurate Effective-One-Body waveforms of inspiralling and coalescing black-hole binaries
• Enhancing Gravitational-Wave Science with Machine Learning
• Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case
• Analytical determination of the two-body gravitational interaction potential at the 4th post-Newtonian approximation
• Search for gravitational waves from binary inspirals in S3 and S4 LIGO data
• Energetics of two-body Hamiltonians in post-Minkowskian gravity
• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• Gravitational Wave Astronomy: in Anticipation of First Sources to be Detected
• Modeling gravitational radiation from coalescing binary black holes
• An improved analysis of GW150914 using a fully spin-precessing waveform model
• Testing post-Newtonian theory with gravitational wave observations
• Periastron Advance in Black-Hole Binaries
• Equivalence between the ADM-Hamiltonian and the harmonic-coordinates approaches to the third post-Newtonian dynamics of compact binaries
• Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
• Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-precessing, spinning, equal-mass black holes
• High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
• Gravitational Waves from Quasicircular Extreme Mass-Ratio Inspirals as Probes of Scalar-Tensor Theories
• Spinning-black-hole scattering and the test-black-hole limit at second post-Minkowskian order
• Gravitational Recoil during Binary Black Hole Coalescence using the Effective One Body Approach
• Extracting equation of state parameters from black hole-neutron star mergers. I. Nonspinning black holes
• Searching for Gravitational Waves from Compact Binaries with Precessing Spins
• A multipolar effective one body waveform model for spin-aligned black hole binaries
• Faithful Effective-One-Body waveforms of equal-mass coalescing black-hole binaries
• Conservative dynamics of two-body systems at the fourth post-Newtonian approximation of general relativity
• The complete non-spinning effective-one-body metric at linear order in the mass ratio
• Binary black holes in circular orbits. I. A global spacetime approach
• Search for Gravitational Waves from Low Mass Binary Coalescences in the First Year of LIGO's S5 Data
• Anatomy of the binary black hole recoil: A multipolar analysis
• Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
• Black-hole Spectroscopy by Making Full Use of Gravitational-Wave Modeling
• Frequency-domain P-approximant filters for time-truncated inspiral gravitational wave signals from compact binaries
• Extracting equation of state parameters from black hole-neutron star mergers: aligned-spin black holes and a preliminary waveform model
• The final spin from the coalescence of aligned-spin black-hole binaries
• Error-analysis and comparison to analytical models of numerical waveforms produced by the NRAR Collaboration
• The Distribution of Recoil Velocities from Merging Black Holes
• Gravitational radiation reaction along general orbits in the effective one-body formalism
• Gravitational self-force and the effective-one-body formalism between the innermost stable circular orbit and the light ring
• On the mass radiated by coalescing black-hole binaries
• Analytic modelling of tidal effects in the relativistic inspiral of binary neutron stars
• Exploring the Bayesian parameter estimation of binary black holes with LISA
• Testing gravitational-wave searches with numerical relativity waveforms: Results from the first Numerical INJection Analysis (NINJA) project
• Effects of waveform model systematics on the interpretation of GW150914
• Tests of General Relativity with GWTC-3
• Precession effect of the gravitational self-force in a Schwarzschild spacetime and the effective one-body formalism
• Implications of Eccentric Observations on Binary Black Hole Formation Channels
• Effective field theory calculation of conservative binary dynamics at third post-Newtonian order
• Binary black hole merger in the extreme mass ratio limit
• The Science Case for LIGO-India
• Mergers of nonspinning black-hole binaries: Gravitational radiation characteristics
• Accurate numerical simulations of inspiralling binary neutron stars and their comparison with effective-one-body analytical models
• Beyond the geodesic approximation: conservative effects of the gravitational self-force in eccentric orbits around a Schwarzschild black hole
• Quasiuniversal properties of neutron star mergers
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
• Tidal Effects in the Post-Minkowskian Expansion
• Universality in the classical limit of massless gravitational scattering
• Classical Gravitational Scattering at $\mathcal{O}(G^3)$ from Feynman Diagrams
• Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings
• GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot }$
• Minding the gap: GW190521 as a straddling binary
• Mergers of binary neutron stars with realistic spin
• A template bank to search for gravitational waves from inspiralling compact binaries I: physical models
• Gravitational Waves: Sources, Detectors and Searches
• A tapering window for time-domain templates and simulated signals in the detection of gravitational waves from coalescing compact binaries
• Electromagnetic Counterparts to Massive Black Hole Mergers
• Radiative contributions to gravitational scattering
• Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections
• Eccentric binary black-hole mergers: The transition from inspiral to plunge in general relativity
• Constraints on quasi-normal-mode frequencies with LIGO-Virgo binary-black-hole observations
• Strong-Field Scattering of Two Black Holes: Numerics Versus Analytics
• Hamiltonian formulation of general relativity and post-Newtonian dynamics of compact binaries
• Detection of IMBHs with ground-based gravitational wave observatories: A biography of a binary of black holes, from birth to death
• Formation of the Black Holes in the Highest Redshift Quasars
• Quadratic-in-Spin Hamiltonian at $\mathcal{O}(G^2)$ from Scattering Amplitudes
• Leading Nonlinear Tidal Effects and Scattering Amplitudes
• Reducing orbital eccentricity of precessing black-hole binaries
• Gravitational self-force corrections to two-body tidal interactions and the effective one-body formalism
• Five-Loop Static Contribution to the Gravitational Interaction Potential of Two Point Masses
• Overspinning a Kerr black hole: the effect of self-force
• On the properties of the massive binary black hole merger GW170729
• Impact of Higher Harmonics in Searching for Gravitational Waves from Non-Spinning Binary Black Holes
• Galaxy bulges and their massive black holes: a review
• A physical template family for gravitational waves from precessing binaries of spinning compact objects: Application to single-spin binaries
• Gravitational waves from inspiralling compact binaries: hexagonal template placement and its efficiency in detecting physical signals
• Search for gravitational waves from binary black hole inspirals in LIGO data
• Spin effects on gravitational waves from inspiraling compact binaries at second post-Newtonian order
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Extreme Mass-Ratio Inspirals in the Effective-One-Body Approach: Quasi-Circular, Equatorial Orbits around a Spinning Black Hole
• Numerical relativity reaching into post-Newtonian territory: a compact-object binary simulation spanning 350 gravitational-wave cycles
• Circular orbits of corotating binary black holes: comparison between analytical and numerical results
• Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
• Parameter estimation with gravitational waves
• Plunge waveforms from inspiralling binary black holes
• The Science of the Einstein Telescope
• Effective-one-body waveforms for precessing coalescing compact binaries with post-newtonian Twist
• The Overlap of Numerical Relativity, Perturbation Theory and Post-Newtonian Theory in the Binary Black Hole Problem
• High-order post-Newtonian contributions to the two-body gravitational interaction potential from analytical gravitational self-force calculations
• Exploring tidal effects of coalescing binary neutron stars in numerical relativity
• Gravitational scattering of two black holes at the fourth post-Newtonian approximation
• The Sub-Leading Scattering Waveform from Amplitudes
• Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger
• Binary black hole merger in the extreme-mass-ratio limit: a multipolar analysis
• Gravitational spin-orbit coupling in binary systems at the second post-Minkowskian approximation
• Universal Properties of Light Rings for Stationary Axisymmetric Spacetimes
• Gravitational Self-Force Correction to the Innermost Stable Circular Equatorial Orbit of a Kerr Black Hole
• Fourth post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach
• An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations
• Effective-one-body waveforms from dynamical captures in black hole binaries
• Gravitational spin-orbit coupling in binary systems, post-Minkowskian approximation and effective one-body theory
• Energy versus Angular Momentum in Black Hole Binaries
• Constraining the evolutionary history of Newton's constant with gravitational wave observations
• Gravitational self-torque and spin precession in compact binaries
• Listening to the Universe with Gravitational-Wave Astronomy
• Modeling multipolar gravitational-wave emission from small mass-ratio mergers
• Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates
• Effective one body Hamiltonian of two spinning black-holes with next-to-next-to-leading order spin-orbit coupling
• Radiation-reaction force and multipolar waveforms for eccentric, spin-aligned binaries in the effective-one-body formalism
• Hydrodynamic Simulations in 3+1 General Relativity
• Energetics and phasing of nonprecessing spinning coalescing black hole binaries
• Small mass plunging into a Kerr black hole: Anatomy of the inspiral-merger-ringdown waveforms
• The Effect of Massive Perturbers on Extreme Mass-Ratio Inspiral Waveforms
• Null infinity waveforms from extreme-mass-ratio inspirals in Kerr spacetime
• A new analytic representation of the ringdown waveform of coalescing spinning black hole binaries
• Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• Second post-Newtonian gravitational wave polarizations for compact binaries in elliptical orbits
• Binary black hole coalescence in the large-mass-ratio limit: the hyperboloidal layer method and waveforms at null infinity
• Binary black hole coalescence in the extreme-mass-ratio limit: testing and improving the effective-one-body multipolar waveform
• A higher-multipole gravitational waveform model for an eccentric binary black holes based on the effective-one-body-numerical-relativity formalism
• Waveform systematics in the gravitational-wave inference of tidal parameters and equation of state from binary neutron star signals
• Recoil velocity at 2PN order for spinning black hole binaries
• Parameterized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method
• A tale of two exponentiations in $\mathcal{N}=8$ supergravity at subleading level
• Numerical Relativity of Compact Binaries in the 21st Century
• Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries
• Nonlinear-in-spin effects in effective-one-body waveform models of spin-aligned, inspiralling, neutron star binaries
• Rush the inspiral: efficient Effective One Body time-domain gravitational waveforms
• Two-body gravitational spin-orbit interaction at linear order in the mass ratio
• Canonical Hamiltonian for an extended test body in curved spacetime: To quadratic order in spin
• Binary black hole merger gravitational waves and recoil in the large mass ratio limit
• The numerical relativity breakthrough for binary black holes
• Effect of calibration errors on Bayesian parameter estimation for gravitational wave signals from inspiral binary systems in the advanced detectors era
• Spin effects on neutron star fundamental-mode dynamical tides: phenomenology and comparison to numerical simulations
• A quasi-physical family of gravity-wave templates for precessing binaries of spinning compact objects: Application to double-spin precessing binaries
• A hybrid post-Newtonian -- effective-one-body scheme for spin-precessing compact-binary waveforms
• Final spin of a coalescing black-hole binary: an Effective-One-Body approach
• Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
• Gravitational waves at the first post-Newtonian order with the Weyssenhoff fluid in Einstein-Cartan theory
• Accuracy of the Post-Newtonian Approximation: Optimal Asymptotic Expansion for Quasi-Circular, Extreme-Mass Ratio Inspirals
• Scattering of tidally interacting bodies in post-Minkowskian gravity
• Radiated momentum in the Post-Minkowskian worldline approach via reverse unitarity
• Coalescence of black hole--neutron star binaries
• The dynamics of precessing binary black holes using the post-Newtonian approximation
• Mining the Geodesic Equation for Scattering Data
• Binary black hole initial data for numerical general relativity based on post-Newtonian data
• The Current Status of Binary Black Hole Simulations in Numerical Relativity
• Periastron advance in spinning black hole binaries: comparing effective-one-body and Numerical Relativity
• First Law of Mechanics for Compact Binaries on Eccentric Orbits
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• Gravitational waves from black hole collisions via an eclectic approach
• Importance of transient resonances in extreme-mass-ratio inspirals
• Modelling the final state from binary black-hole coalescences
• Breakdown of the classical double copy for the effective action of dilaton-gravity at NNLO
• Accuracy and effectualness of closed-form, frequency-domain waveforms for non-spinning black hole binaries
• Modeling the horizon-absorbed gravitational flux for equatorial-circular orbits in Kerr spacetime
• Template banks to search for low-mass binary black holes in advanced gravitational-wave detectors
• Systematic biases in parameter estimation of binary black-hole mergers
• Comprehensive numerical relativity -- effective-one-body comparison to inform improvements in waveform models for binary neutron star systems
• Next-to-next-to-leading order post-Newtonian spin(1)-spin(2) Hamiltonian for self-gravitating binaries
• Conservative self-force correction to the innermost stable circular orbit: comparison with multiple post-Newtonian-based methods
• Hairy binary black holes in Einstein-Maxwell-dilaton theory and their effective-one-body description
• Horizon-absorption effects in coalescing black-hole binaries: An effective-one-body study of the non-spinning case
• Signatures of extra dimensions in gravitational waves from black hole quasi-normal modes
• Accuracy and precision of gravitational-wave models of inspiraling neutron star -- black hole binaries with spin: comparison with numerical relativity in the low-frequency regime
• First Law of Mechanics for Black Hole Binaries with Spins
• Gravitational waveforms from SpEC simulations : neutron star-neutron star and low-mass black hole-neutron star binaries
• Test black holes, scattering amplitudes and perturbations of Kerr spacetime
• NR/HEP: roadmap for the future
• Comparison Between Self-Force and Post-Newtonian Dynamics: Beyond Circular Orbits
• Towards a Non-singular Paradigm of Black Hole Physics
• Relevance of tidal effects and post-merger dynamics for binary neutron star parameter estimation
• Exciting black hole modes via misaligned coalescences: I. Inspiral, transition, and plunge trajectories using a generalized Ori-Thorne procedure
• 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
• Machine Learning Gravitational Waves from Binary Black Hole Mergers
• Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence: Further investigations
• 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
• Introductory lectures on the Effective One Body formalism
• 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
• An efficient filter for detecting gravitational wave bursts in interferometric detectors
• Confirming and improving post-Newtonian and effective-one-body results from self-force computations along eccentric orbits around a Schwarzschild black hole
• Pseudospectrum and binary black hole merger transients
• Status of black-hole-binary simulations for gravitational-wave detection
• Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
• Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code
• The SXS Collaboration's third catalog of binary black hole simulations
• 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
• Improving gravitational-wave parameter estimation using Gaussian process regression
• Extreme mass ratio inspirals on the equatorial plane in the adiabatic order
• Reliability of complete gravitational waveform models for compact binary coalescences
• Denoising of gravitational wave signals via dictionary learning algorithms
• On the Neutron Star-Black Hole Binaries Produced by Binary-driven-Hypernovae
• 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
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• 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
• A Precessing Numerical Relativity Waveform Surrogate Model for Binary Black Holes: A Gaussian Process Regression Approach
• 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
• Comparison of post-Minkowskian and self-force expansions: Scattering in a scalar charge toy model
• Measuring precession in asymmetric compact binaries
• Dynamical Determination of the Innermost Stable Circular Orbit of Binary Neutron Stars
• Measuring intermediate mass black hole binaries with advanced gravitational wave detectors
• 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
• On the four-loop static contribution to the gravitational interaction potential of two point masses
• New Avenue for Accurate Analytical Waveforms and Fluxes for Eccentric Compact Binaries
• Relativistic orbits around spinning supermassive black holes. Secular evolution to 4.5 post-Newtonian order
• Analytical Black-Hole Binary Merger Waveforms
• Towards a gravitational self force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• Strong-field scattering of two spinning black holes: Numerics versus Analytics
• A Rosetta Stone for eccentric gravitational waveform models
• Gravitational radiation from compact binary systems in Einstein-Maxwell-dilaton theories
• LIGO GW150914 and GW151226 Gravitational Wave Detection and Generalized Gravitation Theory (MOG)
• Uncertainty in hybrid gravitational waveforms: Optimizing initial orbital frequencies for binary black-hole simulations
• New gravitational self-force analytical results for eccentric orbits around a Schwarzschild black hole
• Constraints on the binary black hole nature of GW151226 and GW170608 from the measurement of spin-induced quadrupole moments
• Comparing Effective One Body Hamiltonians for spin-aligned coalescing binaries
• 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
• Horizon radiation reaction forces
• Two-body problem in Scalar-Tensor theories as a deformation of General Relativity : an Effective-One-Body approach
• 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
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Impact of Numerical Relativity information on effective-one-body waveform models
• Spin-orbit precession along eccentric orbits for extreme mass ratio black hole binaries and its effective-one-body transcription
• Third post-Newtonian effective-one-body Hamiltonian in scalar-tensor and Einstein-scalar-Gauss-Bonnet gravity
• Mode coupling of Schwarzschild perturbations: Ringdown frequencies
• Spin contributions to the gravitational-waveform modes for spin-aligned binaries at the 3.5PN order
• Gravitomagnetic tidal effects in gravitational waves from neutron star binaries
• On modeling for Kerr black holes: Basis learning, QNM frequencies, and spherical-spheroidal mixing coefficients
• The Kepler equation for inspiralling compact binaries
• Horizon-absorbed energy flux in circularized, nonspinning black-hole binaries and its effective-one-body representation
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• An effective action model of dynamically scalarizing binary neutron stars
• Transition from adiabatic inspiral to plunge into a spinning black hole
• Searching for ringdown higher modes with a numerical relativity-informed post-merger model
• Calabi-Yau meets Gravity: A Calabi-Yau three-fold at fifth post-Minkowskian order
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• Spin-dependent two-body interactions from gravitational self-force computations
• The General Relativistic Two Body Problem and the Effective One Body Formalism
• Numerical simulations of black-hole binaries and gravitational wave emission
• Radiative losses and radiation-reaction effects at the first post-Newtonian order in Einstein-Cartan theory
• Prospects for Measuring the Hubble Constant with Neutron-Star-Black-Hole Mergers
• Interpreting the results of searches for gravitational waves from coalescing binaries
• New Kludge Scheme for the Construction of Approximate Waveforms for Extreme-Mass-Ratio Inspirals
• Multi-waveform inference of gravitational waves
• Modelling gravitational waves from precessing black-hole binaries: Progress, challenges and prospects
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals
• High post-Newtonian order gravitational self-force analytical results for eccentric orbits around a Kerr black hole
• Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order
• Intermediate-mass-ratio-inspirals in the Einstein Telescope. II. Parameter estimation errors
• Redshift factor and the first law of binary black hole mechanics in numerical simulations
• Numerical computation of the EOB potential q using self-force results
• Quasi-5.5PN TaylorF2 approximant for compact binaries: point-mass phasing and impact on the tidal polarizability inference
• Intermediate-mass-ratio-inspirals in the Einstein Telescope: I. Signal-to-noise ratio calculations
• 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
• Gauge Invariant Perturbations of General Spherically Symmetric Spacetimes
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Post-Minkowskian Theory Meets the Spinning Effective-One-Body Approach for Two-Body Scattering
• First gravitational-wave search for intermediate-mass black hole mergers with higher order harmonics
• Fourth post-Newtonian effective-one-body Hamiltonians with generic spins
• A new effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
• Stability of nonspinning effective-one-body model in approximating two-body dynamics and gravitational-wave emission
• Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
• Quasi-equilibrium Binary Black Hole Initial Data for Dynamical Evolutions
• Renormalizing Love: tidal effects at the third post-Newtonian order
• Greybody Factors Imprinted on Black Hole Ringdowns. II. Merging Binary Black Holes
• On the detectability of higher harmonics with LISA
• Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
• Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
• Gravitational Waveforms for Precessing, Quasicircular Compact Binaries with Multiple Scale Analysis: Small Spin Expansion
• The Black Hole Remnant of Black Hole-Neutron Star Coalescing Binaries
• Binary black hole spacetimes with a helical Killing vector
• Exploring waveforms with non-GR deviations for extreme mass-ratio inspirals
• Tidal interaction in binary black hole inspiral
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• Numerical black hole initial data with low eccentricity based on post-Newtonian orbital parameters
• Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral
• Ringdown amplitudes of nonspinning eccentric binaries
• Numerical-relativity validation of effective-one-body waveforms in the intermediate-mass-ratio regime
• Fast post-adiabatic waveforms in the time domain: Applications to compact binary coalescences in LIGO and Virgo
• GRB 140619B: a short GRB from a binary neutron star merger leading to black hole formation
• Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM
• Self-force framework for transition-to-plunge waveforms
• Parameter estimation of coalescing supermassive black hole binaries with LISA
• Remodeling the Effective One-Body Formalism in Post-Minkowskian Gravity
• Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
• Gravitational waves from spinning binary black holes at the leading post-Newtonian orders at all orders in spin
• Gravitational Bound Waveforms from Amplitudes
• Post-Newtonian Waveforms from Spinning Scattering Amplitudes
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• New self-consistent effective one-body theory for spinless binaries based on the post-Minkowskian approximation
• Self-consistent adiabatic inspiral and transition motion
• Gyroscope precession along bound equatorial plane orbits around a Kerr black hole
• Constraining the spin parameter of near-extremal black holes using LISA
• Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods
• Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling for two nonprecessing black holes with aligned spins
• Conservative second-order gravitational self-force on circular orbits and the effective one-body formalism
• Including mode mixing in a higher-multipole model for gravitational waveforms from nonspinning black-hole binaries
• Self-consistent Effective-one-body theory for spinless binaries based on post-Minkowskian approximation I: Hamiltonian and decoupled equation for ${\psi }_4^B$
• Binary mergers in strong gravity background of Kerr black hole
• Searching for near-horizon quantum structures in the binary black-hole stochastic gravitational-wave background
• Self-force effects on the marginally bound zoom-whirl orbit in Schwarzschild spacetime
• Quasi-stationary binary inspiral II: Radiation-balanced boundary conditions
• Deep Generative Models of Gravitational Waveforms via Conditional Autoencoder
• Spin-orbit precession along eccentric orbits: improving the knowledge of self-force corrections and of their effective-one-body counterparts
• Self-consistent effective-one-body theory for spinning binaries based on post-Minkowskian approximation
• Ineffectiveness of Padé resummation techniques in post-Newtonian approximations
• The antikick strikes back: recoil velocities for nearly-extremal binary black hole mergers in the test-mass limit
• High-accuracy waveforms for black hole-neutron star systems with spinning black holes
• Template Banks for Binary black hole searches with Numerical Relativity waveforms
• Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals from Black-hole Perturbation Approach
• Classifying post-Minkowskian geometries for gravitational waves via loop-by-loop Baikov
• Gravitoelectric dynamical tides at second post-Newtonian order
• Horizon Surface Gravity in Corotating Black Hole Binaries
• High-accuracy simulations of highly spinning binary neutron star systems
• Binary black hole detection rates in inspiral gravitational wave searches
• Hybrid method for understanding black-hole mergers: Inspiralling case
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Post-Newtonian templates for gravitational waves from compact binary inspirals
• Understanding binary neutron star collisions with hypermodels
• Effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Self-gravitating ring of matter in orbit around a black hole: The innermost stable circular orbit
• Nonlocal-in-time effective one body Hamiltonian in scalar-tensor gravity at third post-Newtonian order
• Impact of eccentricity and mean anomaly in numerical relativity mergers
• Dynamics around supermassive black holes: Extreme mass-ratio inspirals as gravitational-wave sources
• Analytic toy-model for the ISCO shift
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• Analytical effective-one-body formalism for extreme-mass-ratio inspirals: eccentric orbits
• Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
• Phenomenology and origin of late-time tails in eccentric binary black hole mergers
• Transition from inspiral to plunge into a highly spinning black hole
• 2.5PN accurate waveform information for generic-planar-orbit binaries in effective one-body models
• Deep Learning Model on Gravitational Waveforms in Merging and Ringdown Phases of Binary Black Hole Coalescences
• Spinning compact binary dynamics and chameleon orbits
• Scattering Amplitudes and N-Body Post-Minkowskian Hamiltonians in General Relativity and Beyond
• Gravitational radiation close to a black hole horizon: Waveform regularization and the out-going echo
• A hybrid method for understanding black-hole mergers: head-on case
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• The H-graph with equal masses in terms of multiple polylogarithms
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• New class of post-Newtonian approximants to the waveform templates of inspiralling compact binaries: Test-mass in the Schwarzschild spacetime
• New gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole: redshift invariant
• Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
• Excitation of high frequency voices from intermediate-mass-ratio inspirals with large eccentricity
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Testing gravity with Extreme-Mass-Ratio Inspirals
• Dynamical quasinormal mode excitation
• Late-time tails in nonlinear evolutions of merging black holes
• A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity
• Spin and Quadrupole Couplings for High Spin Equatorial Intermediate Mass-ratio Coalescences
• Geometrized effective-one-body formalism for extreme-mass-ratio limits: Generic orbits
• Reduction of the two-body dynamics to a one-body description in classical electrodynamics
• Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models
• Signal based vetoes for the detection of gravitational waves from inspiralling compact binaries
• Multipolar gravitational waveforms and ringdowns generated during the plunge from the innermost stable circular orbit into a Schwarzschild black hole
• Detecting transient gravitational waves in non-Gaussian noise with partially redundant analysis methods
• Strong Field Scattering of Black Holes: Assessing Resummation Strategies
• Frankenstein's Glue: Transition functions for approximate solutions
• Detweiler's redshift invariant for spinning particles along circular orbits on a Schwarzschild background
• New gravitational self-force analytical results for eccentric equatorial orbits around a Kerr black hole: gyroscope precession
• Post-adiabatic waveform-generation framework for asymmetric precessing binaries
• Accurate modeling of intermediate-mass-ratio inspirals: Exploring the form of the self-force in the intermediate-mass-ratio regime
• Gravitational Waves versus X and Gamma Ray Emission in a Short Gamma-Ray Burst
• Gravitational Wavetrains in the Quasi-Equilibrium Approximation: A Model Problem in Scalar Gravitation
• Premerger phenomena in neutron-star binary coalescences
• A template bank to search for gravitational waves from inspiralling compact binaries: II. Phenomenological model
• 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
• Searching for binary coalescences with inspiral templates: Detection and parameter estimation
• Charged test-particle scattering and effective one-body metrics with spin
• An independent search of gravitational waves in the first observation run of advanced LIGO using cross-correlation
• Detweiler's redshift invariant for extended bodies orbiting a Schwarzschild black hole
• Ballistic orbits in Schwarzschild space-time and gravitational waves from EMR binary mergers
• Fast Evolution and Waveform Generator for Extreme-Mass-Ratio Inspirals in Equatorial-Circular Orbits
• Detectability of gravitational higher order modes in the third-generation era
• SCoRe: A New Framework to Study Unmodeled Physics from Gravitational Wave Data
• Black hole binary inspiral and trajectory dominance
• Merger states and final states of black hole coalescences: a numerical-relativity-assisted effective-one-body approach
• The First Detection of Gravitational Waves
• Real modes and null memory contributions in effective-one-body models
• Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
• An effective-gravity perspective on the Sun-Jupiter-comet three-body system
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• 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
• Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models
• Astronomy and astrophysics with gravitational waves in the Advanced Detector Era
• Schwarzschild Fuzzball and Explicitly Unitary Hawking Radiations
• Novel Screening with Two Bodies: Summing the ladder in disformal scalar-tensor theories
• Peaking into the abyss: Characterizing the merger of equatorial-eccentric-geodesic plunges in rotating black holes
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• Binary black holes in Mkns as sources of gravitational radiation for space based interferometers
• Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
• Approach to the separatrix with eccentric orbits
• Gravitational waves in massive gravity: Waveforms generated by a particle plunging into a black hole and the excitation of quasinormal modes and quasibound states
• High-energy hyperbolic scattering by neutron stars and black holes
• Classification of Feynman integral geometries for black-hole scattering at 5PM order
• Effective metric of spinless binaries with radiation-reaction effect up to fourth Post-Minkowskian order in effective-one-body theory
• More about scalar gravity
• The Design Strain Sensitivity of the Schenberg Spherical Resonant Antenna for Gravitational Waves
• Highly accurate simulations of asymmetric black-hole scattering and cross validation of effective-one-body models
• Waveforms from Amplitudes
• Gravitational self-force corrections to tidal invariants for spinning particles on circular orbits in a Schwarzschild spacetime
• Gravitational self-force corrections to tidal invariants for particles on eccentric orbits in a Schwarzschild spacetime
• Electromagnetic absorption, emission and scattering spectra of black holes with tidal charge
• Waveforms produced by a scalar point particle plunging into a Schwarzschild black hole: Excitation of quasinormal modes and quasibound states
• Transition-to-plunge self-force waveforms with a spinning primary
• Mother templates for gravitational wave chirps
• Prospects for intermediate mass black hole binary searches with advanced gravitational-wave detectors
• Electromagnetic radiation generated by a charged particle plunging into a Schwarzschild black hole: Multipolar waveforms and ringdowns
• Analytical determination of the periastron advance in spinning binaries from self-force computations
• Gravitational self-force corrections to tidal invariants for particles on circular orbits in a Kerr spacetime
• Testing the Boundary-to-Bound Correspondence with Numerical Relativity
• Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
• Numerical relativity simulations in the era of the Einstein Telescope
• Astrophysics with the Laser Interferometer Space Antenna
• Binary Black Hole Coalescence in Semi-Analytic Puncture Evolution
• Gravitational Waves from Stellar Black Hole Binaries and the Impact on Nearby Sun-like Stars
• Energy flux and waveforms by coalescing spinless binary system in effective one-body theory
• Gravitational-wave searches in the era of Advanced LIGO and Virgo
• Solar system dynamics in general relativity
• Scattering of uncharged particles in the field of two extremely charged black holes
• The first law of binary black hole scattering
• Testing the validity of the phenomenological gravitational waveform models for nonspinning binary black hole searches at low masses
• The general relativistic two body problem
• Search for gravitational waves from eccentric binary black holes with an effective-one-body template
• Success of the small mass ratio approximation during the final orbits of binary black hole simulations
• Observable Signatures of EMRI Black Hole Binaries Embedded in Thin Accretion Disks
• Extreme Mass-Ratio Binary Black Hole Merger: Characteristics of the Test-Particle Limit
• Signatures of a spinning supermassive black hole binary on the mas-scale jet of the quasar S5 1928+738 based on 25 years of VLBI data
• Probing Particle Physics with Gravitational Waves
• Arrival Times of Gravitational Radiation Peaks for Binary Inspiral
• The Effective One Body description of the Two-Body problem
• An Effective Field Theory for Binary Cosmic Strings
• Report on the first binary black hole inspiral search in LIGO data
• The gravitational two-body problem in the vicinity of the light ring: Insights from the black-hole-ring toy model
• Advancing the Effective-One-Body Framework in the Test-Mass Limit
• Ringdown of a postinnermost stable circular orbit of a rapidly spinning black hole: Mass ratio dependence of higher harmonic quasinormal mode excitation
• Black-Hole Perturbation Plus Post-Newtonian Theory: Hybrid Waveform for Neutron Star Binaries
• Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
• Estimating the Final Spin of Binary Black Holes Merger in STU Supergravity
• Dynamics for Super-Extremal Kerr Binary Systems at $\mathcal{O}(G^2)$
• Binary superradiance: a numerical study
• Eccentric Pairs: Analytic Gravitational Waves from Binary Black Holes in Elliptic Orbits
• Gravitational waveform model based on photon motion for spinning black holes
• Merging Black Holes: Assessing the Performance of Two Analytic Gravitational Waves Models
• Strong Field Scattering of Two Black Holes: Exploring Gauge Flexibility
• Gravitational scattering of two neutron stars
• A full waveform model for arbitrarily axis-symmetric black hole mergers
• Black Hole and Neutron Star Binaries: Theoretical Challenges
• Waveform models for the gravitational-wave memory effect: Extreme mass-ratio limit and final memory offset
• Preparations for detecting and characterizing gravitational-wave signals from binary black hole coalescences
• The Eikonal Approximation and the Gravitational Dynamics of Binary Systems
• Microscopic State of BHs and an Exact One Body Method for Binary Dynamics in General Relativity
• Asymptotically matched quasi-circular inspiral and transition-to-plunge in the small mass ratio expansion
• Analysis of late-time tails in spin-aligned eccentric binary black hole mergers
• Gravitational-wave signatures of nonviolent nonlocality
• Constants of motion in gravitational self-force theory
• 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
• The Radial Action from Probe Amplitudes to All Orders
• Compact binary system dynamics at the second post-Newtonian order: analytical formula of the coordinate time for eccentric and circular orbits
• Scattering Amplitudes for Binary Systems beyond GR
• First-post-Newtonian generation of gravitational waves in Einstein-Cartan theory
• Conditional Autoencoder for Generating Binary Neutron Star Waveforms with Tidal and Precession Effects
• Marginally bound circular orbits in the composed black-hole-ring system
• Three models of non-perturbative quantum-gravitational binding
• 2.5PN kick from black-hole binaries in circular orbit: Nonspinning case
• Rising Tides: Analytic Modeling of Tidal Effects in Binary Neutron Star Mergers
• Hybrid waveforms for precessing quasi-circular binary systems
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Analytical solutions of bound timelike geodesic orbits in effective-one-body frame
• Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries
• Assessment of Effective-One-Body Radiation Reactions for Generic Planar Orbits
• Waveforms and fluxes: Towards a self-consistent effective one body waveform model for nonprecessing, coalescing black-hole binaries for third generation detectors
• Learning Post-Newtonian Corrections from Numerical Relativity
• Comparing eccentric waveform models based on post-Newtonian and effective-one-body approaches, over an observationally relevant parameter space
• Energetics and scattering of gravitational two-body systems at fourth post-Minkowskian order
• Search for gravitational waves from binary black hole inspiral, merger and ringdown
• Effective-one-body formalism for leading-order radiative effects in the post-linear framework
• Early Warning From Eccentric Compact Binaries: Template Initialization And Sub-dominant Mode Effects
• Precisely computing bound orbits of spinning bodies around black holes I: General framework and results for nearly equatorial orbits
• Black hole sensitivities in Einstein-scalar-Gauss-Bonnet gravity
• AthenaK simulations of the binary black hole merger GW150914