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Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes

文献类型：期刊论文

作者Belczynski, K.14; Klencki, J.15; Fields, C. E.16; Olejak, A.17,18; Berti, E.19; Meynet, G.20; Fryer, C. L.25; Holz, D. E.24; O'Shaughnessy, R.21; Brown, D. A.22
刊名ASTRONOMY & ASTROPHYSICS
出版日期2020-04-24
卷号636页码:40
ISSN号0004-6361
关键词stars: massive black hole physics gravitational waves
DOI10.1051/0004-6361/201936528
英文摘要All ten LIGO/Virgo binary black hole (BH-BH) coalescences reported following the O1/O2 runs have near-zero effective spins. There are only three potential explanations for this. If the BH spin magnitudes are large, then: (i) either both BH spin vectors must be nearly in the orbital plane or (ii) the spin angular momenta of the BHs must be oppositely directed and similar in magnitude. Then there is also the possibility that (iii) the BH spin magnitudes are small. We consider the third hypothesis within the framework of the classical isolated binary evolution scenario of the BH-BH merger formation. We test three models of angular momentum transport in massive stars: a mildly efficient transport by meridional currents (as employed in the Geneva code), an efficient transport by the Tayler-Spruit magnetic dynamo (as implemented in the MESA code), and a very-efficient transport (as proposed by Fuller et al.) to calculate natal BH spins. We allow for binary evolution to increase the BH spins through accretion and account for the potential spin-up of stars through tidal interactions. Additionally, we update the calculations of the stellar-origin BH masses, including revisions to the history of star formation and to the chemical evolution across cosmic time. We find that we can simultaneously match the observed BH-BH merger rate density and BH masses and BH-BH effective spins. Models with efficient angular momentum transport are favored. The updated stellar-mass weighted gas-phase metallicity evolution now used in our models appears to be key for obtaining an improved reproduction of the LIGO/Virgo merger rate estimate. Mass losses during the pair-instability pulsation supernova phase are likely to be overestimated if the merger GW170729 hosts a BH more massive than 50 M-circle dot. We also estimate rates of black hole-neutron star (BH-NS) mergers from recent LIGO/Virgo observations. If, in fact. angular momentum transport in massive stars is efficient, then any (electromagnetic or gravitational wave) observation of a rapidly spinning BH would indicate either a very effective tidal spin up of the progenitor star (homogeneous evolution, high-mass X-ray binary formation through case A mass transfer, or a spin- up of a Wolf-Rayet star in a close binary by a close companion), significant mass accretion by the hole, or a BH formation through the merger of two or more BHs (in a dense stellar cluster).
WOS关键词GRAVITATIONAL-WAVE SOURCES ; ROTATING MASSIVE STARS ; GAMMA-RAY BURSTS ; M-CIRCLE-DOT ; STELLAR EVOLUTION ; NEUTRON-STARS ; PRESUPERNOVA EVOLUTION ; DIFFERENT METALLICITIES ; DIFFERENTIAL ROTATION ; GALACTIC DISTRIBUTION
资助项目Polish National Science Center (NCN) grant Maestro[2018/30/A/ST9/00050] ; NCN grant OPUS[2015/19/B/ST9/01099] ; Netherlands Organisation for Scientific Research (NWO) ; Edward J Petry Graduate Fellowship from Michigan State University ; National Science Foundation Graduate Research Fellowship Program[DGE1424871] ; National Science Centre, Poland[UMO-2016/23/B/ST9/02732] ; EU COST Action[CA16117] ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust[RPG-2019-350] ; NASA through Einstein Postdoctoral Fellowship[PF6-170152] ; NASA[NAS8-03060] ; NASA[80NSSC18K0527] ; Polish National Science Center (NCN) Grant[UMO-2014/14/M/ST9/00707] ; NSF[PHY-1607130] ; NSF[AST-1716715] ; NSF[AST-1412449] ; NSF[PHY-1505629] ; NSF[PHY-1607520] ; NSF[PHY-1708081] ; FCT under the IF2014 Programme[IF/00797/2014/CP1214/CT0012] ; Swiss National Science Foundation[200020-160119] ; National Science Foundation[PHY-1404395] ; National Science Foundation[NSF PHY-1748958] ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences[2018PM0017] ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe[XDB23040000] ; Carl Tryggers Foundation for Scientific Research[CTS 17:113] ; KITP UC Santa Barbara ; French Space Agency CNES ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Marion and Stuart Rice Award ; DNRF ; [HST-AR-15021.001-A]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者EDP SCIENCES S A
WOS记录号WOS:000530118400001
资助机构Polish National Science Center (NCN) grant Maestro ; Polish National Science Center (NCN) grant Maestro ; NCN grant OPUS ; NCN grant OPUS ; Netherlands Organisation for Scientific Research (NWO) ; Netherlands Organisation for Scientific Research (NWO) ; Edward J Petry Graduate Fellowship from Michigan State University ; Edward J Petry Graduate Fellowship from Michigan State University ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; National Science Centre, Poland ; National Science Centre, Poland ; EU COST Action ; EU COST Action ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust ; Leverhulme Trust ; NASA through Einstein Postdoctoral Fellowship ; NASA through Einstein Postdoctoral Fellowship ; NASA ; NASA ; Polish National Science Center (NCN) Grant ; Polish National Science Center (NCN) Grant ; NSF ; NSF ; FCT under the IF2014 Programme ; FCT under the IF2014 Programme ; Swiss National Science Foundation ; Swiss National Science Foundation ; National Science Foundation ; National Science Foundation ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Carl Tryggers Foundation for Scientific Research ; Carl Tryggers Foundation for Scientific Research ; KITP UC Santa Barbara ; KITP UC Santa Barbara ; French Space Agency CNES ; French Space Agency CNES ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Marion and Stuart Rice Award ; Marion and Stuart Rice Award ; DNRF ; DNRF ; Polish National Science Center (NCN) grant Maestro ; Polish National Science Center (NCN) grant Maestro ; NCN grant OPUS ; NCN grant OPUS ; Netherlands Organisation for Scientific Research (NWO) ; Netherlands Organisation for Scientific Research (NWO) ; Edward J Petry Graduate Fellowship from Michigan State University ; Edward J Petry Graduate Fellowship from Michigan State University ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; National Science Centre, Poland ; National Science Centre, Poland ; EU COST Action ; EU COST Action ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust ; Leverhulme Trust ; NASA through Einstein Postdoctoral Fellowship ; NASA through Einstein Postdoctoral Fellowship ; NASA ; NASA ; Polish National Science Center (NCN) Grant ; Polish National Science Center (NCN) Grant ; NSF ; NSF ; FCT under the IF2014 Programme ; FCT under the IF2014 Programme ; Swiss National Science Foundation ; Swiss National Science Foundation ; National Science Foundation ; National Science Foundation ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Carl Tryggers Foundation for Scientific Research ; Carl Tryggers Foundation for Scientific Research ; KITP UC Santa Barbara ; KITP UC Santa Barbara ; French Space Agency CNES ; French Space Agency CNES ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Marion and Stuart Rice Award ; Marion and Stuart Rice Award ; DNRF ; DNRF ; Polish National Science Center (NCN) grant Maestro ; Polish National Science Center (NCN) grant Maestro ; NCN grant OPUS ; NCN grant OPUS ; Netherlands Organisation for Scientific Research (NWO) ; Netherlands Organisation for Scientific Research (NWO) ; Edward J Petry Graduate Fellowship from Michigan State University ; Edward J Petry Graduate Fellowship from Michigan State University ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; National Science Centre, Poland ; National Science Centre, Poland ; EU COST Action ; EU COST Action ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust ; Leverhulme Trust ; NASA through Einstein Postdoctoral Fellowship ; NASA through Einstein Postdoctoral Fellowship ; NASA ; NASA ; Polish National Science Center (NCN) Grant ; Polish National Science Center (NCN) Grant ; NSF ; NSF ; FCT under the IF2014 Programme ; FCT under the IF2014 Programme ; Swiss National Science Foundation ; Swiss National Science Foundation ; National Science Foundation ; National Science Foundation ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Carl Tryggers Foundation for Scientific Research ; Carl Tryggers Foundation for Scientific Research ; KITP UC Santa Barbara ; KITP UC Santa Barbara ; French Space Agency CNES ; French Space Agency CNES ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Marion and Stuart Rice Award ; Marion and Stuart Rice Award ; DNRF ; DNRF ; Polish National Science Center (NCN) grant Maestro ; Polish National Science Center (NCN) grant Maestro ; NCN grant OPUS ; NCN grant OPUS ; Netherlands Organisation for Scientific Research (NWO) ; Netherlands Organisation for Scientific Research (NWO) ; Edward J Petry Graduate Fellowship from Michigan State University ; Edward J Petry Graduate Fellowship from Michigan State University ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; National Science Centre, Poland ; National Science Centre, Poland ; EU COST Action ; EU COST Action ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Centre Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust ; Leverhulme Trust ; NASA through Einstein Postdoctoral Fellowship ; NASA through Einstein Postdoctoral Fellowship ; NASA ; NASA ; Polish National Science Center (NCN) Grant ; Polish National Science Center (NCN) Grant ; NSF ; NSF ; FCT under the IF2014 Programme ; FCT under the IF2014 Programme ; Swiss National Science Foundation ; Swiss National Science Foundation ; National Science Foundation ; National Science Foundation ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Strategic Priority Research Program of the Chinese Academy of Science Multiwaveband Gravitational Wave Universe ; Carl Tryggers Foundation for Scientific Research ; Carl Tryggers Foundation for Scientific Research ; KITP UC Santa Barbara ; KITP UC Santa Barbara ; French Space Agency CNES ; French Space Agency CNES ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Kavli Institute for Cosmological Physics at the University of Chicago through Kavli Foundation ; Marion and Stuart Rice Award ; Marion and Stuart Rice Award ; DNRF ; DNRF
源URL[http://ir.bao.ac.cn/handle/114a11/55174]  
专题中国科学院国家天文台
通讯作者Belczynski, K.
作者单位1.Univ Maryland, Joint Space Sci Inst, College Pk, MD 20742 USA
2.Univ Maryland, Dept Astron, College Pk, MD 20742 USA
3.Keele Univ, Lennard Jones Labs, Keele ST5 5BG, Staffs, England
4.Univ Birmingham, Sch Phys & Astron, Birmingham, W Midlands, England
5.Univ Birmingham, Inst Gravitat Wave Astron, Birmingham, W Midlands, England
6.Lund Univ, Dept Astron & Theoret Phys, Lund Observ, Box 43, S-22100 Lund, Sweden
7.Kenyon Coll, Dept Phys, 201 North Coll RD, Gambier, OH 43022 USA
8.SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
9.Natl Astron Observ, Beijing, Peoples R China
10.Univ Chinese Acad Sci, Beijing, Peoples R China
推荐引用方式
GB/T 7714		 Belczynski, K.,Klencki, J.,Fields, C. E.,et al. Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes[J]. ASTRONOMY & ASTROPHYSICS,2020,636:40.
APA Belczynski, K..,Klencki, J..,Fields, C. E..,Olejak, A..,Berti, E..,...&Lasota, J. -P..(2020).Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes.ASTRONOMY & ASTROPHYSICS,636,40.
MLA Belczynski, K.,et al."Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes".ASTRONOMY & ASTROPHYSICS 636(2020):40.

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