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Mapping the asymptotic inspiral of precessing binary black holes to their merger remnants

Reali, Luca and Mould, Matthew and Gerosa, Davide and Varma, Vijay (2020) Mapping the asymptotic inspiral of precessing binary black holes to their merger remnants. Classical and Quantum Gravity, 37 (22). Art. No. 225005. ISSN 0264-9381. https://resolver.caltech.edu/CaltechAUTHORS:20201021-122915698

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Abstract

Multiple approaches are required to study the evolution of black-hole binaries. While the post-Newtonian (PN) approximation is sufficient to describe the early inspiral (even from infinitely large orbital separation), only numerical relativity can capture the full complexity of the dynamics near merger. We combine multi-timescale PN integrations with numerical-relativity surrogate models, thus mapping the entire history of the binary from its asymptotic configuration at past-time infinity to the post-merger remnant. This approach naturally allows us to assess the impact of the precessional and orbital phase on the properties—mass, spin, and kick—of the merger remnant. These phases introduce a fundamental uncertainty when connecting the two extrema of the binary evolution.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1088/1361-6382/abb639DOIArticle
https://arxiv.org/abs/2005.01747arXivDiscussion Paper
ORCID:
AuthorORCID
Reali, Luca0000-0002-8143-6767
Mould, Matthew0000-0001-5460-2910
Gerosa, Davide0000-0002-0933-3579
Varma, Vijay0000-0002-9994-1761
Additional Information:© 2020 IOP Publishing. Received 4 May 2020, revised 2 September 2020; Accepted for publication 8 September 2020; Published 16 October 2020. We thank Michael Kesden, Ulrich Sperhake, and Emanuele Berti for discussions. LR is supported by the ERC H2020 project HPC-EUROPA3 (INFRAIA-2016-1-730897). DG is supported by Leverhulme Trust Grant No. RPG-2019-350. Computational work was performed at the Edinburgh Parallel Computing Center (EPCC), the University of Birmingham BlueBEAR cluster, the Athena cluster at HPC Midlands + funded by EPSRC Grant No. EP/P020232/1, and the Maryland Advanced Research Computing Center (MARCC).
Group:TAPIR
Funders:
Funding AgencyGrant Number
European Research Council (ERC)INFRAIA-2016-1-730897
Leverhulme TrustRPG-2019-350
Engineering and Physical Sciences Research Council (EPSRC)EP/P020232/1
Subject Keywords:black holes, gravitational waves, numerical relativity, relativistic astrophysics
Issue or Number:22
Record Number:CaltechAUTHORS:20201021-122915698
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201021-122915698
Official Citation:Luca Reali et al 2020 Class. Quantum Grav. 37 225005
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106186
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Oct 2020 19:35
Last Modified:21 Oct 2020 19:35

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