Rapid Stellar and Binary Population Synthesis with COMPAS

被引：95

作者：

Riley, Jeff ^{[1
,2
]}

Agrawal, Poojan ^{[2
,3
]}

Barrett, Jim W. ^{[4
,5
]}

Boyett, Kristan N. K. ^{[6
]}

Broekgaarden, Floor S. ^{[7
]}

Chattopadhyay, Debatri ^{[2
,3
]}

Gaebel, Sebastian M. ^{[8
]}

Gittins, Fabian ^{[9
,10
]}

Hirai, Ryosuke ^{[1
,2
]}

Howitt, George ^{[2
,11
]}

Justham, Stephen ^{[12
,13
,14
,15
]}

Khandelwal, Lokesh ^{[12
,13
]}

Kummer, Floris ^{[12
,13
]}

Lau, Mike Y. M. ^{[1
,2
]}

Mandel, Ilya ^{[1
,2
,4
,5
]}

de Mink, Selma E. ^{[7
,12
,13
,15
]}

Neijssel, Coenraad ^{[2
,4
,5
]}

Riley, Tim ^{[1
,2
]}

van Son, Lieke ^{[7
,12
,13
,15
]}

Stevenson, Simon ^{[2
,3
]}

Vigna-Gomez, Alejandro ^{[16
,17
]}

Vinciguerra, Serena ^{[2
,4
,5
]}

Wagg, Tom ^{[7
,15
,18
]}

Willcox, Reinhold ^{[1
,2
]}

机构：

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

[2] Australian Res Council, OzGrav, Ctr Excellence Gravitat Wave Discovery, Hawthorn, Vic, Australia

[3] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

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

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

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

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

[8] Max Planck Inst Gravitat Phys, Albert Einstein Inst, Callinstr 38, D-30167 Hannover, Germany

[9] Univ Southampton, Math Sci, Southampton SO17 1BJ, Hants, England

[10] Univ Southampton, STAG Res Ctr, Southampton SO17 1BJ, Hants, England

[11] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia

[12] Anton Pannekoek Inst Astron, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[13] GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[14] Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100012, Peoples R China

[15] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany

[16] Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvei 128, DK-2200 Copenhagen, Denmark

[17] Niels Bohr Int Acad, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark

[18] Univ Washington, Dept Astron, Seattle, WA 98195 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2022年 / 258卷 / 02期

基金：

澳大利亚研究理事会; 美国国家科学基金会; 欧洲研究理事会; 新加坡国家研究基金会;

关键词：

X-RAY BINARIES; COMMON-ENVELOPE EVOLUTION; BLACK-HOLE BINARIES; CHEMICALLY HOMOGENEOUS EVOLUTION; ELECTRON-CAPTURE SUPERNOVAE; CORE-COLLAPSE SUPERNOVAE; ASYMPTOTIC GIANT BRANCH; NEUTRON-STAR ACCRETION; RADIATION-DRIVEN WINDS; DOUBLE WHITE-DWARFS;

D O I：

10.3847/1538-4365/ac416c

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Compact Object Mergers: Population Astrophysics and Statistics (COMPAS; https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of isolated stellar binaries under a set of parameterized assumptions in order to allow comparisons against observational data sets, such as those coming from gravitational-wave observations of merging compact remnants. It includes a number of tools for population processing in addition to the core binary evolution components. COMPAS is publicly available via the GitHub repository https://github.com/TeamCOMPAS/COMPAS/, and is designed to allow for flexible modifications as evolutionary models improve. This paper describes the methodology and implementation of COMPAS. It is a living document that will be updated as new features are added to COMPAS; the current document describes COMPAS v02.21.00.

引用

页数：30

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