Gravitational waveforms for compact binaries from second-order self-force theory

Abstract

We produce gravitational waveforms for nonspinning compact binaries undergoing a quasicircular inspiral. Our approach is based on a two-timescale expansion of the Einstein equations in second-order self-force theory, which allows first-principles waveform production in tens of milliseconds. Although the approach is designed for extreme mass ratios, our waveforms agree remarkably well with those from full numerical relativity, even for comparable-mass systems. Our results will be invaluable in accurately modelling extreme-mass-ratio inspirals for the LISA mission and intermediate-mass-ratio systems currently being observed by the LIGO-Virgo-KAGRA Collaboration.

References in corpus (55)

• Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
• Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
• Self-force and radiation reaction in general relativity
• Surrogate models for precessing binary black hole simulations with unequal masses
• A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
• Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation
• IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
• New Horizons for Fundamental Physics with LISA
• The evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission
• Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides and self-spin effects
• Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
• A Comparison of search templates for gravitational waves from binary inspiral
• Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
• Surrogate model of hybridized numerical relativity binary black hole waveforms
• Enriching the Symphony of Gravitational Waves from Binary Black Holes by Tuning Higher Harmonics
• How black holes get their kicks: Gravitational radiation recoil revisited
• FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis
• The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole
• Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit
• Periastron Advance in Black-Hole Binaries
• The First Law of Binary Black Hole Mechanics in General Relativity and Post-Newtonian Theory
• Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
• Second-order gravitational self-force
• Second-order self-force calculation of the gravitational binding energy in compact binaries
• The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
• Analytic modelling of tidal effects in the relativistic inspiral of binary neutron stars
• Gravitational Self-Force Correction to the Binding Energy of Compact Binary Systems
• Frequency domain reduced order model of aligned-spin effective-one-body waveforms with higher-order modes
• Gravitational-wave energy flux for compact binaries through second order in the mass ratio
• Gravitational waveforms from a point particle orbiting a Schwarzschild black hole
• Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime
• The Head-On Collision of Two Equal Mass Black Holes Peter Anninos
• The Overlap of Numerical Relativity, Perturbation Theory and Post-Newtonian Theory in the Binary Black Hole Problem
• An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole
• Black hole perturbation theory and gravitational self-force
• Nonlinear gravitational self-force: second-order equation of motion
• A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries
• Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries
• A practical, covariant puncture for second-order self-force calculations
• Numerical Relativity of Compact Binaries in the 21st Century
• Nonlinear gravitational self-force. I. Field outside a small body
• Extreme black hole simulations: collisions of unequal mass black holes and the point particle limit
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• Periastron Advance in Spinning Black Hole Binaries: Gravitational Self-Force from Numerical Relativity
• Exciting black hole modes via misaligned coalescences: I. Inspiral, transition, and plunge trajectories using a generalized Ori-Thorne procedure
• Applying the effective-source approach to frequency-domain self-force calculations: Lorenz-gauge gravitational perturbations
• Second-order perturbation theory: problems on large scales
• Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
• Second-order perturbation theory: the problem of infinite mode coupling
• Applying the effective-source approach to frequency-domain self-force calculations
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• Slow evolution of the metric perturbation due to a quasicircular inspiral into a Schwarzschild black hole
• Semi-analytic expressions for quasinormal modes of slowly rotating Kerr black holes
• Gravitational recoil in nonspinning black hole binaries: the span of test-mass results
• Horizon Surface Gravity in Corotating Black Hole Binaries

Cited by in corpus (82)

• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
• The Science of the Einstein Telescope
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• Gravitational-Wave Phasing of Quasi-Circular Compact Binary Systems to the Fourth-and-a-Half post-Newtonian Order
• Extreme mass-ratio inspirals into black holes surrounded by scalar clouds
• Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning Compact Binaries to the Fourth Post-Newtonian Order
• Extreme mass-ratio inspirals in ultra-light dark matter
• Effective Field Theory for Extreme Mass Ratios
• Fast and Fourier: Extreme Mass Ratio Inspiral Waveforms in the Frequency Domain
• Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• Extreme mass-ratio inspiral and waveforms for a spinning body into a Kerr black hole via osculating geodesics and near-identity transformations
• 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
• Inspiral-inherited ringdown tails
• ESIGMAHM: An Eccentric, Spinning inspiral-merger-ringdown waveform model with Higher Modes for the detection and characterization of binary black holes
• Analytic solutions for the motion of spinning particles near spherically symmetric black holes and exotic compact objects
• Self-force framework for transition-to-plunge waveforms
• Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity
• Impact of relativistic waveforms in LISA's science objectives with extreme-mass-ratio inspirals
• Spinning particles near Kerr black holes: Orbits and gravitational-wave fluxes through the Hamilton-Jacobi formalism
• Amplitudes and Polarizations of Quadratic Quasi-Normal Modes for a Schwarzschild Black Hole
• Self-forced inspirals with spin-orbit precession
• Metric perturbations of Kerr spacetime in Lorenz gauge: Circular equatorial orbits
• Detecting Strong Gravitational Lensing of Gravitational Waves with TianQin
• Extreme mass ratio inspirals in rotating dark matter spikes
• Applying the effective-source approach to frequency-domain self-force calculations for eccentric orbits
• Probing fundamental physics with Extreme Mass Ratio Inspirals: a full Bayesian inference for scalar charge
• Testing gravity with Extreme-Mass-Ratio Inspirals
• Gravitational memory: new results from post-Newtonian and self-force theory
• Late-time tails in nonlinear evolutions of merging black holes
• Influence of mass-ratio corrections in extreme-mass-ratio inspirals for testing general relativity
• Implementation of a GHZ-Teukolsky puncture scheme for gravitational self-force calculations
• Post-adiabatic waveform-generation framework for asymmetric precessing binaries
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Actions of spinning compact binaries: Spinning particle in Kerr matched to dynamics at 1.5 post-Newtonian order
• Second-order gravitational self-force in a highly regular gauge: Covariant and coordinate punctures
• Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation
• Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT
• Multi-domain spectral method for self-force calculations
• Interplay between numerical relativity and perturbation theory : finite size effects
• Worldtube excision method for intermediate-mass-ratio inspirals: scalar-field model in 3+1 dimensions
• Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
• Resonant excitation of eccentricity in spherical extreme-mass-ratio inspirals
• EMRI_MC: A GPU-based Python code for Bayesian inference of EMRI waveforms
• Transition-to-plunge self-force waveforms with a spinning primary
• Sourced metric perturbations of Kerr spacetime in Lorenz gauge
• Complete quasinormal modes of Type-D black holes
• Gravitational wave fluxes on generic orbits in near-extreme Kerr spacetime: higher spin and large eccentricity
• Assessing the systematic errors of extreme-mass-ratio inspirals waveforms for testing general relativity
• Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole
• Inferring Binary Properties from Gravitational Wave Signals
• Improving the scalability of Gaussian-process error marginalization in gravitational-wave inference
• Interplay between numerical-relativity and black hole perturbation theory in the intermediate-mass-ratio regime
• Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary
• Toward Second-Order Self-Force for Eccentric Extreme-Mass Ratio Inspirals in Schwarzschild Spacetime
• Gravitational waves from quasielliptic compact binaries in scalar-tensor theory to one-and-a-half post-Newtonian order
• Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism
• On the approximate relation between black-hole perturbation theory and numerical relativity
• Systematic errors in fast relativistic waveforms for Extreme Mass Ratio Inspirals
• Building a bridge between comparable and extreme mass ratio black hole binaries: a single spin precessing model for the final state
• Simple, efficient method of calculating the Detweiler-Whiting singular field to very high order
• The first law of binary black hole scattering
• A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
• Black-hole scattering with numerical relativity: Self-force extraction and post-Minkowskian validation
• Analytic solutions for the motion of spinning particles near brane-world black hole
• A note on the conversion of orbital angles for extreme mass ratio inspirals
• Post-Newtonian expansion of fluxes from a scalar charge on an inclined-spherical orbit about a Kerr black hole
• Waveform models for the gravitational-wave memory effect: Extreme mass-ratio limit and final memory offset
• Relieving scale disparity in binary black hole simulations
• Constants of motion in gravitational self-force theory
• Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries
• GW250114 reveals black hole horizon signatures
• Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications
• Metric reconstruction and the Hamiltonian for eccentric, precessing binaries in the small-mass-ratio limit
• Secular evolution of orbital parameters for general bound orbits in Kerr spacetime
• Hybrid waveforms for precessing quasi-circular binary systems
• Generic effective sources for first-order in mass-ratio gravitational self-force calculations in Schwarzschild spacetime
• Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals
• Comparing numerical relativity and perturbation theory waveforms for a non-spinning equal-mass binary
• Particles with precessing spin in Kerr spacetime: analytic solutions for eccentric orbits and homoclinic motion near the equatorial plane
• Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries