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Full 3D numerical relativity simulations of neutron star–boson star collisions with BAM

Abstract:

With the first direct detections of gravitational waves (GWs) from the coalescence of compact binaries observed by the advanced LIGO and VIRGO interferometers, the era of GW astronomy has begun. Whilst there is strong evidence that the observed GWs are connected to the merger of two black holes (BH) or two neutron stars (NS), future detections may present a less consistent picture. Indeed, the possibility that the observed GW signal was created by a merger of exotic compact objects (ECOs) suc...

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Publication status:
Published
Peer review status:
Peer reviewed

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Files:
Publisher copy:
10.1088/1361-6382/aaf43e

Authors


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Role:
Author
ORCID:
0000-0003-2374-307X
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Sub department:
Astrophysics
Department:
Unknown
Role:
Author
ORCID:
0000-0001-8841-1522
Publisher:
Institute of Physics
Journal:
Classical and Quantum Gravity More from this journal
Volume:
36
Issue:
2
Article number:
025002
Publication date:
2018-12-18
Acceptance date:
2018-11-27
DOI:
EISSN:
1361-6382
ISSN:
0264-9381
Pubs id:
pubs:954603
UUID:
uuid:fb849ab8-d62c-4ec9-bb95-f2ef8978f9bb
Local pid:
pubs:954603
Source identifiers:
954603
Deposit date:
2018-12-23

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