Cosmic rates of black hole mergers and pair-instability supernovae from chemically homogeneous binary evolution

被引：87

作者：

du Buisson, L. ^{[1
]}

Marchant, P. ^{[2
]}

Podsiadlowski, Ph ^{[1
,3
]}

Kobayashi, C. ^{[4
]}

Abdalla, F. B. ^{[5
]}

Taylor, P. ^{[6
,7
]}

Mandel, I ^{[7
,8
,9
,10
]}

de Mink, S. E. ^{[11
,12
]}

Moriya, T. J. ^{[8
,13
]}

Langer, N. ^{[3
]}

机构：

[1] Univ Oxford, Dept Phys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England

[2] Katholieke Univ Leuven, Inst Astron, Celestijnenlaan 200 D, B-3001 Leuven, Belgium

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

[4] Univ Hertfordshire, Ctr Astrophys Res, Dept Phys Astron & Math, Hatfield AL10 9AB, Herts, England

[5] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[6] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia

[7] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, 1 Turner Ave,Brodie Hall Bldg,Technol Pk, Bentley, WA 6102, Australia

[8] Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia

[9] Swinburne Univ Technol, ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Level 9 AMDC Bldg, Hawthorn, Vic 3122, Australia

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

[11] Harvard Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[12] Univ Amsterdam, Anton Pannekoek Inst Astron, NL-1090 GE Amsterdam, Netherlands

[13] Natl Inst Nat Sci, Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 2211, Japan

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2020年 / 499卷 / 04期

基金：

欧盟地平线“2020”; 英国科学技术设施理事会; 澳大利亚研究理事会; 美国国家科学基金会; 日本学术振兴会;

关键词：

gravitational waves; stars: interiors; stars: mass-loss; supernovae: general; galaxies: star formation; NEUTRON-STAR; METALLICITY DEPENDENCE; GALACTIC DISTRIBUTION; MASSIVE STARS; PULSAR; PROSPECTS; PROGENITORS; CONSTRAINTS; COALESCENCE; PREDICTIONS;

D O I：

10.1093/mnras/staa3225

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

During the first three observing runs of the Advanced gravitational-wave detector network, the LIGO/Virgo collaboration detected several black hole binary (BHBH) mergers. As the population of detected BHBH mergers grows, it will become possible to constrain different channels for their formation. Here we consider the chemically homogeneous evolution (CHE) channel in close binaries, by performing population synthesis simulations that combine realistic binary models with detailed cosmological calculations of the chemical and star-formation history of the Universe. This allows us to constrain population properties, as well as cosmological and aLIGO/aVirgo detection rates of BHBH mergers formed through this pathway. We predict a BHBH merger rate at redshift zero of 5.8 Gpc(-3)yr(-1) through the CHE channel, to be compared with aLIGO/aVirgo's measured rate of 53.2(-28.)(2+55.8) Gpc(-3)yr(-1), and find that eventual merger systems have BH masses in the range 17-43 M-circle dot below the pair-instability supernova (PISN) gap, and >124 M-circle dot above the PISN gap. We investigate effects of momentum kicks during black hole formation, and calculate cosmological and magnitude limited PISN rates. We also study the effects of high-redshift deviations in the star formation rate. We find that momentum kicks tend to increase delay times of BHBH systems, and our magnitude limited PISN rate estimates indicate that current deep surveys should be able to detect such events. Lastly, we find that our cosmological merger rate estimates change by at most similar to 8 per cent for mild deviations of the star formation rate in the early Universe, and by up to similar to 40 per cent for extreme deviations.

引用

页码：5941 / 5959

页数：19

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