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On the formation history of Galactic double neutron stars

文献类型：期刊论文

作者Vigna-Gomez, Alejandro1,2,3; Neijssel, Coenraad J.1,2; Stevenson, Simon1,2,4; Barrett, Jim W.1,2; Belczynski, Krzysztof5; Justham, Stephen3,6,7,8; de Mink, Selma E.8; Mueller, Bernhard9; Podsiadlowski, Philipp3,10; Renzo, Mathieu8
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2018-12-01
卷号481期号:3页码:4009-4029
关键词binaries: general stars: neutron pulsars: general
ISSN号0035-8711
DOI10.1093/mnras/sty2463
英文摘要Double neutron stars (DNSs) have been observed as Galactic radio pulsars, and the recent discovery of gravitational waves from the DNS merger GW170817 adds to the known DNS population. We perform rapid population synthesis of massive binary stars and discuss model predictions, including DNS formation rates, mass distributions, and delay time distributions. We vary assumptions and parameters of physical processes such as mass transfer stability criteria, supernova natal kick distributions, remnant mass prescriptions, and common-envelope energetics. We compute the likelihood of observing the orbital period-eccentricity distribution of the Galactic DNS population under each of our population synthesis models, allowing us to quantitatively compare the models. We find that mass transfer from a stripped post-helium-burning secondary (case BB) on to a neutron star is most likely dynamically stable. We also find that a natal kick distribution composed of both low (Maxwellian sigma = 30 km s(-1)) and high (sigma = 265 km s(-1)) components is preferred over a single high-kick component. We conclude that the observed DNS mass distribution can place strong constraints on model assumptions.
WOS关键词ELECTRON-CAPTURE SUPERNOVAE ; GAMMA-RAY BURSTS ; MASSIVE CLOSE BINARIES ; COMPACT OBJECT MERGER ; BLACK-HOLE ; POPULATION SYNTHESIS ; CORE-COLLAPSE ; CONSTRAINING POPULATION ; STELLAR EVOLUTION ; COALESCENCE RATES
资助项目Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; PHAROS European Cooperation in Science and Technology (COST) Action[CA16214] ; Science and Technology Facilities Council (STFC) ; Polish National Science Center (NCN)[DEC-2012/07/E/ST9/01360] ; Polish National Science Center (NCN)[2015/19/B/ST9/01099] ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe'[XDB23040000] ; Chinese Academy of Sciences[2011Y2JB07] ; National Natural Science Foundation of China[11633005] ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC)[GS100010663] ; National Science Foundation[NSF PHY11-25915] ; Australian Research Council (ARC) through ARC Future Fellowship[FT160100035] ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery[CE170100004] ; Kavli Foundation ; Danish National Research Foundation (DNRF)
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000450984100083
出版者OXFORD UNIV PRESS
资助机构Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; PHAROS European Cooperation in Science and Technology (COST) Action ; PHAROS European Cooperation in Science and Technology (COST) Action ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; National Science Foundation ; National Science Foundation ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Kavli Foundation ; Kavli Foundation ; Danish National Research Foundation (DNRF) ; Danish National Research Foundation (DNRF) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; PHAROS European Cooperation in Science and Technology (COST) Action ; PHAROS European Cooperation in Science and Technology (COST) Action ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; National Science Foundation ; National Science Foundation ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Kavli Foundation ; Kavli Foundation ; Danish National Research Foundation (DNRF) ; Danish National Research Foundation (DNRF) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; PHAROS European Cooperation in Science and Technology (COST) Action ; PHAROS European Cooperation in Science and Technology (COST) Action ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; National Science Foundation ; National Science Foundation ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Kavli Foundation ; Kavli Foundation ; Danish National Research Foundation (DNRF) ; Danish National Research Foundation (DNRF) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; PHAROS European Cooperation in Science and Technology (COST) Action ; PHAROS European Cooperation in Science and Technology (COST) Action ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Sciences 'Multi-waveband Gravitational Wave Universe' ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; National Science Foundation ; National Science Foundation ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council (ARC) through ARC Future Fellowship ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery ; Kavli Foundation ; Kavli Foundation ; Danish National Research Foundation (DNRF) ; Danish National Research Foundation (DNRF)
源URL[http://ir.bao.ac.cn/handle/114a11/23636]  
专题中国科学院国家天文台
通讯作者Vigna-Gomez, Alejandro
作者单位1.Univ Birmingham, Birmingham Inst Gravitat Wave Astron, Birmingham B15 2TT, W Midlands, England
2.Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
3.Univ Copenhagen, Niels Bohr Inst, DARK, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
4.Swinburne Univ Technol, OzGrav, Hawthorn, Vic 3122, Australia
5.Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland
6.Univ Chinese Acad Sci, Space Sci, Sch Astron, Beijing 100012, Peoples R China
7.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
8.Univ Amsterdam, Anton Pannekoek Inst Astron, NL-1090 GE Amsterdam, Netherlands
9.Monash Univ, Monash Ctr Astrophys, Sch Phys & Astron, Clayton, Vic 3800, Australia
10.Univ Oxford, Dept Astron, Oxford OX1 3RH, England
推荐引用方式
GB/T 7714		 Vigna-Gomez, Alejandro,Neijssel, Coenraad J.,Stevenson, Simon,et al. On the formation history of Galactic double neutron stars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,481(3):4009-4029.
APA Vigna-Gomez, Alejandro.,Neijssel, Coenraad J..,Stevenson, Simon.,Barrett, Jim W..,Belczynski, Krzysztof.,...&Mandel, Ilya.(2018).On the formation history of Galactic double neutron stars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,481(3),4009-4029.
MLA Vigna-Gomez, Alejandro,et al."On the formation history of Galactic double neutron stars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 481.3(2018):4009-4029.

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