Tail-induced spin-orbit effect in the gravitational radiation of compact binaries

Abstract

Gravitational waves contain tail effects which are due to the back-scattering of linear waves in the curved space-time geometry around the source. In this paper we improve the knowledge and accuracy of the two-body inspiraling post-Newtonian (PN) dynamics and gravitational-wave signal by computing the spin-orbit terms induced by tail effects. Notably, we derive those terms at 3PN order in the gravitational-wave energy flux, and 2.5PN and 3PN orders in the wave polarizations. This is then used to derive the spin-orbit tail effects in the phasing through 3PN order. Our results can be employed to carry out more accurate comparisons with numerical-relativity simulations and to improve the accuracy of analytical templates aimed at describing the whole process of inspiral, merger and ringdown.

Minor corrections. To be published in Physical Review D

References in corpus (12)

• Higher-order spin effects in the dynamics of compact binaries I. Equations of motion
• Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-spinning, equal-mass black holes
• An improved analytical description of inspiralling and coalescing black-hole binaries
• Hamiltonian of two spinning compact bodies with next-to-leading order gravitational spin-orbit coupling
• The Hyperfine Einstein-Infeld-Hoffmann Potential
• Search for gravitational waves from binary inspirals in S3 and S4 LIGO data
• Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-precessing, spinning, equal-mass black holes
• Next-to-leading order gravitational spin-orbit coupling in an effective field theory approach
• ADM canonical formalism for gravitating spinning objects
• Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order
• Higher-order-in-spin interaction Hamiltonians for binary black holes from Poincaré invariance
• Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals

Cited by in corpus (68)

• A simple model of complete precessing black-hole-binary gravitational waveforms
• Tests of General Relativity with GW170817
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
• I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics
• The Effective Field Theorist's Approach to Gravitational Dynamics
• Inspiral-merger-ringdown waveforms of spinning, precessing black-hole binaries in the effective-one-body formalism
• Systematic parameter errors in inspiraling neutron star binaries
• Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
• Constructing Gravitational Waves from Generic Spin-Precessing Compact Binary Inspirals
• Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order
• Next-to-next-to-leading order spin-orbit effects in the gravitational wave flux and orbital phasing of compact binaries
• Ready-to-use post-Newtonian gravitational waveforms for binary black holes with non-precessing spins: An update
• Next-to-next-to-leading order spin-orbit effects in the near-zone metric and precession equations of compact binaries
• The complete non-spinning effective-one-body metric at linear order in the mass ratio
• The tail effect in gravitational radiation-reaction: time non-locality and renormalization group evolution
• Binary dynamics from spin1-spin2 coupling at fourth post-Newtonian order
• Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings
• Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order
• Gravitational Waves from Quasi-Circular Black Hole Binaries in Dynamical Chern-Simons Gravity
• Next-to-next-to-leading order spin-orbit effects in the equations of motion of compact binary systems
• Spin effects on gravitational waves from inspiraling compact binaries at second post-Newtonian order
• Equivalence of ADM Hamiltonian and Effective Field Theory approaches at next-to-next-to-leading order spin1-spin2 coupling of binary inspirals
• Constraining the orbital eccentricity of inspiralling compact binary systems with Advanced LIGO
• Accurate gravitational waveforms for binary-black-hole mergers with nearly extremal spins
• The Overlap of Numerical Relativity, Perturbation Theory and Post-Newtonian Theory in the Binary Black Hole Problem
• Next-to-next-to-leading order gravitational spin-orbit coupling via the effective field theory for spinning objects in the post-Newtonian scheme
• Spinning test-body orbiting around Schwarzschild black hole: circular dynamics and gravitational-wave fluxes
• Next-to-next-to-leading order post-Newtonian linear-in-spin binary Hamiltonians
• Next-to-leading tail-induced spin-orbit effects in the gravitational radiation flux of compact binaries
• Gravitational radiation from inspiralling compact objects: Spin-spin effects completed at the next-to-leading post-Newtonian order
• 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
• N${}^3$LO gravitational spin-orbit coupling at order $G^4$
• Statistical and systematic errors for gravitational-wave inspiral signals: A principal component analysis
• NNNLO gravitational quadratic-in-spin interactions at the quartic order in G
• Asymptotic gravitational wave fluxes from a spinning particle in circular equatorial orbits around a rotating black hole
• Accuracy of gravitational waveform models for observing neutron-star--black-hole binaries in Advanced LIGO
• Fast Frequency-domain Waveforms for Spin-Precessing Binary Inspirals
• Spin effects in gravitational waveforms and fluxes for binaries on eccentric orbits to the third post-Newtonian order
• Gravitational Waveforms for Precessing, Quasi-circular Binaries via Multiple Scale Analysis and Uniform Asymptotics: The Near Spin Alignment Case
• 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
• Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity
• Spin contributions to the gravitational-waveform modes for spin-aligned binaries at the 3.5PN order
• Impact of the second order self-forces on the dephasing of the gravitational waves from quasi-circular extreme mass-ratio inspirals
• On the validity of the adiabatic approximation in compact binary inspirals
• Testing the multipole structure and conservative dynamics of compact binaries using gravitational wave observations: The spinning case
• Tidal interaction in compact binaries: a post-Newtonian affine framework
• Deviation of quadrupolar bodies from geodesic motion in a Kerr spacetime
• Gravitational Waveforms for Precessing, Quasicircular Compact Binaries with Multiple Scale Analysis: Small Spin Expansion
• Spin effects in Spherical Harmonic Modes of Gravitational Waves from Eccentric Compact Binary Inspirals
• Detecting resonant tidal excitations of Rossby modes in coalescing neutron-star binaries with third-generation gravitational-wave detectors
• Higher-order tail contributions to the energy and angular momentum fluxes in a two-body scattering process
• Analytical effective-one-body formalism for extreme-mass-ratio inspirals: eccentric orbits
• Asymptotic frame selection for binary black hole spacetimes II: Post-Newtonian limit
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Canonical Angles In A Compact Binary Star System With Spinning Components: Approximative Solution Through Next-To-Leading-Order Spin-Orbit Interaction for Circular Orbits
• Analytic approximations, perturbation theory, effective field theory methods and their applications
• Gravitational spin-orbit dynamics at the fifth-and-a-half post-Newtonian order
• Tidal contributions to the full gravitational waveform to the second-and-a-half post-Newtonian order
• A Post-Newtonian approach to black hole-fluid systems
• Self-forced evolutions of an implicit rotating source: A natural framework to model comparable and intermediate mass-ratio systems from inspiral through ringdown
• Analytic Solutions to Compact Binary Inspirals With Leading Order Spin-Orbit Contribution Using The Dynamical Renormalization Group
• Octupolar test of general relativity
• Eccentric Motion of Spinning Compact Binaries
• Parametrized multipolar gravitational waveforms for testing general relativity: Amplitude corrections up to 2PN order
• Gravitational waves from spinning compact object binaries: New post-Newtonian results
• Tests of general relativity at the fourth post-Newtonian order
• Eccentricity evolution of spinning binaries and its dependence on the equation of state of the components