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Foundations of an effective-one-body model for coalescing binaries on eccentric orbits

Authors :
Tanja Hinderer
Stanislav Babak
AstroParticule et Cosmologie (APC (UMR_7164))
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
AstroParticule et Cosmologie ( APC - UMR 7164 )
Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA )
Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Source :
Phys.Rev.D, Phys.Rev.D, 2017, 96 (10), pp.104048. ⟨10.1103/PhysRevD.96.104048⟩, Phys.Rev.D, 2017, 96 (10), pp.104048. 〈10.1103/PhysRevD.96.104048〉, Physical Review D, Physical Review D, 96, 1-26, Physical Review D, 96, 10, pp. 1-26
Publication Year :
2017
Publisher :
arXiv, 2017.

Abstract

We develop the foundations of an effective-one-body (EOB) model for eccentric binary coalescences that includes the conservative dynamics, radiation reaction, and gravitational waveform modes from the inspiral and the merger-ringdown signals. We use the same approach as is commonly employed in black-hole perturbation theory by introducing a relativistic parameterization of the dynamics that is defined by the orbital geometry and consists of a set of phase variables and quantities that evolve only due to gravitational radiation reaction. Specializing to nonspinning binaries, we derive the EOB evolution equations and compute the binary's radiative multipole moments that determine the gravitational waves through a decomposition into the fundamental frequencies of the motion. The major differences between our treatment and the quasi-Keplerian approach often used in post-Newtonian (PN) calculations are that the orbital parameters describe strong-field dynamics, and that expressing the multipole moments in terms of the frequencies simplifies the calculations and also results in an unambiguous orbit-averaging operation. While our description of the conservative dynamics is fully relativistic, we limit explicit derivations in the radiative sector to 1.5PN order for simplicity. This already enables us to establish methods for computing both instantaneous and hereditary contributions to the gravitational radiation in EOB coordinates that have straightforward extensions to higher PN order. The weak-field, small eccentricity limit of our results for the orbit-averaged fluxes of energy and angular momentum agrees with known PN results when expressed in terms of gauge-invariant quantities. We further address considerations for the numerical implementation of the model and the completion of the waveforms to include the merger and ringdown signals, and provide illustrative results.<br />Comment: 25 pages, 8 figures, small changes to match published version

Details

ISSN :
24700010
Database :
OpenAIRE
Journal :
Phys.Rev.D, Phys.Rev.D, 2017, 96 (10), pp.104048. ⟨10.1103/PhysRevD.96.104048⟩, Phys.Rev.D, 2017, 96 (10), pp.104048. 〈10.1103/PhysRevD.96.104048〉, Physical Review D, Physical Review D, 96, 1-26, Physical Review D, 96, 10, pp. 1-26
Accession number :
edsair.doi.dedup.....da91697577dc099c6730ed85a48cff0c
Full Text :
https://doi.org/10.48550/arxiv.1707.08426