Effective spin distribution of black hole mergers in triples

Many astrophysical scenarios have been proposed to explain the several black hole (BH) and neutron star binary mergers observed via gravitational waves (GWs) by the LIGO–Virgo collaboration. Contributions from various channels can be statistically disentangled by mass, spin, eccentricity, and redshi...

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Main Authors: Fragione, G, Kocsis
Format: Journal article
Language:English
Published: Oxford University Press 2020
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author Fragione, G
Kocsis
author_facet Fragione, G
Kocsis
author_sort Fragione, G
collection OXFORD
description Many astrophysical scenarios have been proposed to explain the several black hole (BH) and neutron star binary mergers observed via gravitational waves (GWs) by the LIGO–Virgo collaboration. Contributions from various channels can be statistically disentangled by mass, spin, eccentricity, and redshift distributions of merging binaries. In this paper, we investigate the signatures of BH–BH binary mergers induced by a third companion through the Lidov–Kozai mechanism in triple systems. We adopt different prescriptions for the supernovae natal kicks and consider different progenitor metallicities and initial orbital parameters. We show that the typical eccentricity in the LIGO band is 0.01–0.1 and that the merger rate is in the range 0.008−9 Gpc−3 yr−1, depending on the natal kick prescriptions and progenitor metallicity. Furthermore, we find that the typical distribution of effective projected spin is peaked at χeff ∼ 0 with significant tails. We show that the triple scenario could reproduce the distribution of χeff. We find that the triple channel may be strongly constrained by the misalignment angle between the binary component spins in future detections with spin precession.
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spelling oxford-uuid:45a2e7d6-ddf3-48a7-b5f9-eb0769ea591a2022-03-26T15:08:56ZEffective spin distribution of black hole mergers in triplesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:45a2e7d6-ddf3-48a7-b5f9-eb0769ea591aEnglishSymplectic ElementsOxford University Press2020Fragione, GKocsisMany astrophysical scenarios have been proposed to explain the several black hole (BH) and neutron star binary mergers observed via gravitational waves (GWs) by the LIGO–Virgo collaboration. Contributions from various channels can be statistically disentangled by mass, spin, eccentricity, and redshift distributions of merging binaries. In this paper, we investigate the signatures of BH–BH binary mergers induced by a third companion through the Lidov–Kozai mechanism in triple systems. We adopt different prescriptions for the supernovae natal kicks and consider different progenitor metallicities and initial orbital parameters. We show that the typical eccentricity in the LIGO band is 0.01–0.1 and that the merger rate is in the range 0.008−9 Gpc−3 yr−1, depending on the natal kick prescriptions and progenitor metallicity. Furthermore, we find that the typical distribution of effective projected spin is peaked at χeff ∼ 0 with significant tails. We show that the triple scenario could reproduce the distribution of χeff. We find that the triple channel may be strongly constrained by the misalignment angle between the binary component spins in future detections with spin precession.
spellingShingle Fragione, G
Kocsis
Effective spin distribution of black hole mergers in triples
title Effective spin distribution of black hole mergers in triples
title_full Effective spin distribution of black hole mergers in triples
title_fullStr Effective spin distribution of black hole mergers in triples
title_full_unstemmed Effective spin distribution of black hole mergers in triples
title_short Effective spin distribution of black hole mergers in triples
title_sort effective spin distribution of black hole mergers in triples
work_keys_str_mv AT fragioneg effectivespindistributionofblackholemergersintriples
AT kocsis effectivespindistributionofblackholemergersintriples