Symmetry Breaking in Merging Binary Black Holes from Young Massive Clusters and Isolated Binaries

被引：8

作者：

Banerjee, Sambaran ^{[1
,2
]}

Olejak, Aleksandra ^{[3
]}

Belczynski, Krzysztof ^{[3
]}

机构：

[1] Helmholtz Inst Strahlen & Kernphys, Nussallee 14-16, D-53115 Bonn, Germany

[2] Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany

[3] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland

来源：

ASTROPHYSICAL JOURNAL | 2023年 / 953卷 / 01期

关键词：

OPEN STELLAR CLUSTERS; GRAVITATIONAL-WAVES; STAR-CLUSTERS; ALGORITHMIC REGULARIZATION; SPIN MODELS; EVOLUTION; MERGERS; ORIGIN; DYNAMICS; LESSONS;

D O I：

10.3847/1538-4357/acdd59

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Properties of the to-date observed binary black hole (BBH) merger events suggest a preference toward spin-orbit aligned mergers. Naturally, this has caused widespread interest and speculations regarding implications on various merger formation channels. Here we show that (i) not only the BBH merger population from isolated binaries but also (ii) BBH population formed in young massive clusters (YMCs) would possess an asymmetry in favor of aligned mergers, in the distribution of the events' effective spin parameter (& chi; (eff)). In our analysis, we utilize BBH merger outcomes from state-of-the-art N-body evolutionary models of YMCs and isolated binary population synthesis. We incorporate, for the first time in such an analysis, misalignments due to both natal kicks and dynamical encounters. The YMC & chi; (eff) distribution has a mean (an antialigned merger fraction) of & chi; (eff) & LE; 0.04 (f ( X ) - & AP; 40%), which is smaller (larger) than but consistent with the observed asymmetry of & chi; (eff) & AP; 0.06 (f ( X ) - & AP; 28%) as obtained from the population analysis by the LIGO-Virgo-KAGRA collaboration. In contrast, isolated binaries alone tend to produce a much stronger asymmetry; for the tested physical models, & chi; (eff) & AP; 0.25 and f ( X ) - & LSIM; 7%. Although the YMC & chi; (eff) distribution is more similar to the observed counterpart, none of the channels correctly reproduce the observed distribution. Our results suggest that further extensive model explorations for both isolated binary and dynamical channels as well as better observational constraints are necessary to understand the physics of "the symmetry breaking" of the BBH merger population.

引用

页数：16

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