Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond

被引：86

作者：

Baibhav, Vishal ^{[1
]}

Berti, Emanuele ^{[1
]}

Gerosa, Davide ^{[2
,3
]}

Mapelli, Michela ^{[4
,5
,6
,7
]}

Giacobbo, Nicola ^{[4
,5
,6
]}

Bouffanais, Yann ^{[4
,5
]}

Di Carlo, Ugo N. ^{[5
,8
]}

机构：

[1] Johns Hopkins Univ, Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA

[2] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[3] Univ Birmingham, Inst Gravitat Wave Astron, Birmingham B15 2TT, W Midlands, England

[4] Univ Padua, Dipartimenw Fis & Astron Galileo Galilei, Vicolo Osservatorio 3, I-35122 Padua, Italy

[5] INFN, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy

[6] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy

[7] Univ Innsbruck, Inst Astro & Teilchenphys, Technikerstr 25-8, A-6020 Innsbruck, Austria

[8] Univ Insubria, Dipartimento Sci & Alta Tecnol, Via Valleggio 11, I-22100 Como, Italy

来源：

PHYSICAL REVIEW D | 2019年 / 100卷 / 06期

基金：

欧盟地平线“2020”; 欧洲研究理事会;

关键词：

BLACK-HOLE BINARIES; COSMIC MERGER RATE; COMMON-ENVELOPE; NEUTRON-STARS; EVOLUTION; PROGENITORS; METALLICITY; CLUSTERS; IMPACT;

D O I：

10.1103/PhysRevD.100.064060

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using simulations performed with the population synthesis code MOBSE, we compute the merger rate densities and detection rates of compact binary mergers formed in isolation for second- and third-generation gravitational wave detectors. We estimate how rates are affected by uncertainties on key stellar physics parameters, namely common envelope evolution and natal kicks. We estimate how future upgrades will increase the size of the available catalog of merger events, and we discuss features of the merger rate density that will become accessible with third-generation detectors.

引用

页数：8

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