Journal article
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
- 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
Terms of use
- Copyright holder:
- Deme et al.
- Copyright date:
- 2020
- Rights statement:
- Copyright © 2020 The Author(s). Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
- Licence:
- CC Attribution (CC BY)
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