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Detecting Kozai–Lidov imprints on the gravitational waves of intermediate-mass black holes in galactic nuclei

Abstract:
A third object in the vicinity of a binary system causes variations in the eccentricity and the inclination of the binary through the Kozai–Lidov (KL) effect. We examine if such variations leave a detectable imprint on the gravitational waves of a binary consisting of intermediate-mass black holes and stellar-mass objects. As a proof of concept, we present an example where LISA may detect the KL-modulated gravitational wave signals of such sources from at least a distance of 1 Mpc if the perturbation is caused by a supermassive black hole tertiary. Although the quick pericenter precession induced by general relativity significantly reduces the appropriate parameter space for this effect by quenching the KL oscillations, we still find reasonable parameters where the KL effect may be detected with high signal-to-noise ratios.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4357/abafa3

Authors


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Role:
Author
ORCID:
0000-0003-4016-9778
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Role:
Author
ORCID:
0000-0003-0992-0033
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Role:
Author
ORCID:
0000-0002-9802-9279
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Oxford college:
St Hugh's College
Role:
Author
ORCID:
0000-0002-4865-7517


Publisher:
IOP Publishing
Journal:
Astrophysical Journal More from this journal
Volume:
901
Issue:
2
Pages:
125-125
Publication date:
2020-09-29
Acceptance date:
2020-08-11
DOI:
EISSN:
1538-4357
ISSN:
0004-637X


Language:
English
Keywords:
Pubs id:
1136130
Local pid:
pubs:1136130
Deposit date:
2020-10-12

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