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Black hole merger simulations in wave dark matter environments

Abstract:

The interaction of binary black hole mergers with their environments can be studied using numerical relativity simulations. These start only a short finite time before merger, at which point appropriate initial conditions must be imposed. A key task is therefore to identify the configuration that is appropriate for the binary and its environment at this stage of the evolution. In this work we study the behavior of wave dark matter around equal mass black hole binaries, finding that there is a...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1103/PhysRevD.107.024035

Authors


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Role:
Author
ORCID:
0000-0001-7181-3365
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0001-9584-5791
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Oriel College
Role:
Author
ORCID:
0000-0002-3021-2851
Publisher:
American Physical Society
Journal:
Physical Review D More from this journal
Volume:
107
Issue:
2
Article number:
024035
Publication date:
2023-01-15
Acceptance date:
2023-01-13
DOI:
EISSN:
2470-0029
ISSN:
2470-0010
Language:
English
Keywords:
Pubs id:
1329336
Local pid:
pubs:1329336
Deposit date:
2023-03-31

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