Merging hierarchical triple black hole systems with intermediate-mass black holes in population III star clusters

被引:6
作者
Liu, Shuai [1 ,2 ]
Wang, Long [2 ]
Hu, Yi-Ming [2 ]
Tanikawa, Ataru [3 ,4 ]
Trani, Alessandro A. [5 ,6 ,7 ]
机构
[1] Zhaoqing Univ, Sch Elect & Elect Engn, Zhaoqing 526061, Peoples R China
[2] Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China
[3] Univ Tokyo, Coll Arts ans Sci, Dept Earth Sci & Astron, Tokyo 1538902, Japan
[4] Fukui Prefectural Univ, Ctr Informat Sci, Fukui 9101195, Japan
[5] Niels Bohr Inst, Niels Bohr Int Acad, DK-2100 Copenhagen, Denmark
[6] Univ Tokyo, Res Ctr Early Universe, Sch Sci, Tokyo 1130033, Japan
[7] Okinawa Inst Sci & Technol, Okinawa 9040495, Japan
基金
中国博士后科学基金; 中国国家自然科学基金;
关键词
methods: numerical; stars: black holes; stars: Population III; galaxies: star clusters: general; SPACE-TELESCOPE EVIDENCE; MERGER RATE DENSITY; M-CIRCLE-DOT; GRAVITATIONAL-WAVES; RUNAWAY COLLISIONS; FORMATION PATHWAY; NO EVIDENCE; CHIRP MASS; OMEGA CEN; AGN DISCS;
D O I
10.1093/mnras/stae1946
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Theoretical predictions suggest that very massive stars have the potential to form through multiple collisions and eventually evolve into intermediate-mass black holes (IMBHs) within Population III star clusters embedded in mini dark matter haloes. In this study, we investigate the long-term evolution of Population III star clusters, including models with a primordial binary fraction of f(b )= 0 and 1, using the N-body simulation code petar. We comprehensively examine the phenomenon of hierarchical triple black holes in the clusters, specifically focusing on their merging inner binary black holes (BBHs), with post-Newtonian correction, by using the tsunami code. Our findings suggest a high likelihood of the inner BBHs containing IMBHs with masses on the order of O(100)M-circle dot, and as a result, their merger rate could be up to 0.1Gpc(-3)yr(-3). The orbital eccentricities of some merging inner BBHs oscillate over time periodically, known as the Kozai-Lidov oscillation, due to dynamical perturbations. Detectable merging inner BBHs for mHz GW detectors LISA/TianQin/Taiji concentrate within z<3. More distant sources would be detectable for CE/ET/LIGO/KAGRA/DECIGO, which are sensitive from O(0.1)Hz to O(100) Hz. Furthermore, compared with merging isolated BBHs, merging inner BBHs affected by dynamical perturbations from tertiary BHs tend to have higher eccentricities, with a significant fraction of sources with eccentricities closing to 1 at mHz bands. GW observations would help constrain the formation channels of merging BBHs, whether through isolated evolution or dynamical interaction, by examining eccentricities.
引用
收藏
页码:2262 / 2281
页数:20
相关论文
共 169 条
[1]   GW190521: A Binary Black Hole Merger with a Total Mass of 150 M⊙ [J].
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. D. ;
Abraham, S. ;
Acernese, F. ;
Ackley, K. ;
Adams, C. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Allen, G. ;
Allocca, A. ;
Aloy, M. A. ;
Altin, P. A. ;
Amato, A. ;
Anand, S. ;
Ananyeva, A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Angelova, S. V. ;
Antier, S. ;
Appert, S. ;
Arai, K. ;
Araya, M. C. ;
Areeda, J. S. ;
Arene, M. ;
Arnaud, N. ;
Aronson, S. M. ;
Ascenzi, S. ;
Ashton, G. ;
Aston, S. M. ;
Astone, P. ;
Aubin, F. ;
Aufmuth, P. ;
AultONeal, K. ;
Austin, C. ;
Avendano, V. ;
Avila-Alvarez, A. ;
Babak, S. ;
Bacon, P. ;
Badaracco, F. ;
Bader, M. K. M. ;
Bae, S. .
PHYSICAL REVIEW LETTERS, 2020, 125 (10)
[2]   Properties and Astrophysical Implications of the 150 M Binary Black Hole Merger GW190521 [J].
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. D. ;
Abraham, S. ;
Acernese, F. ;
Ackley, K. ;
Adams, C. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Allen, G. ;
Allocca, A. ;
Aloy, M. A. ;
Altin, P. A. ;
Amato, A. ;
Anand, S. ;
Ananyeva, A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Angelova, S. V. ;
Antier, S. ;
Appert, S. ;
Arai, K. ;
Araya, M. C. ;
Areeda, J. S. ;
Arene, M. ;
Arnaud, N. ;
Aronson, S. M. ;
Ascenzi, S. ;
Ashton, G. ;
Aston, S. M. ;
Astone, P. ;
Aubin, F. ;
Aufmuth, P. ;
AultONeal, K. ;
Austin, C. ;
Avendano, V. ;
Avila-Alvarez, A. ;
Babak, S. ;
Bacon, P. ;
Badaracco, F. ;
Bader, M. K. M. ;
Bae, S. .
ASTROPHYSICAL JOURNAL LETTERS, 2020, 900 (01)
[3]   Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network [J].
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. D. ;
Abraham, S. ;
Acernese, F. ;
Ackley, K. ;
Adams, A. ;
Adams, C. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Allen, G. ;
Allocca, A. ;
Aloy, M. A. ;
Altin, P. A. ;
Amato, A. ;
Anand, S. ;
Ananyeva, A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Angelova, S., V ;
Antier, S. ;
Appert, S. ;
Arai, K. ;
Araya, M. C. ;
Areeda, J. S. ;
Arene, M. ;
Arnaud, N. ;
Aronson, S. M. ;
Arun, K. G. ;
Ascenzi, S. ;
Ashton, G. ;
Aston, S. M. ;
Astone, P. ;
Aubin, F. ;
Aufmuth, P. ;
AultONeal, K. ;
Austin, C. ;
Avendano, V ;
Avila-Alvarez, A. ;
Babak, S. ;
Bacon, P. ;
Badaracco, F. .
PHYSICAL REVIEW D, 2019, 100 (06)
[4]   Exploring the sensitivity of next generation gravitational wave detectors [J].
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. D. ;
Abernathy, M. R. ;
Ackley, K. ;
Adams, C. ;
Addesso, P. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Ain, A. ;
Ajith, P. ;
Allen, B. ;
Altin, P. A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Arai, K. ;
Araya, M. C. ;
Arceneaux, C. C. ;
Areeda, J. S. ;
Arun, K. G. ;
Ashton, G. ;
Ast, M. ;
Aston, S. M. ;
Aufmuth, P. ;
Aulbert, C. ;
Babak, S. ;
Baker, P. T. ;
Ballmer, S. W. ;
Barayoga, J. C. ;
Barclay, S. E. ;
Barish, B. C. ;
Barker, D. ;
Barr, B. ;
Barsotti, L. ;
Bartlett, J. ;
Bartos, I. ;
Bassiri, R. ;
Batch, J. C. ;
Baune, C. ;
Bell, A. S. ;
Berger, B. K. ;
Bergmann, G. ;
Berry, C. P. L. ;
Betzwieser, J. ;
Bhagwat, S. ;
Bhandare, R. ;
Bilenko, I. A. .
CLASSICAL AND QUANTUM GRAVITY, 2017, 34 (04)
[5]   GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run [J].
Abbott, R. ;
Abbott, T. D. ;
Acernese, F. ;
Ackley, K. ;
Adams, C. ;
Adhikari, N. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agarwal, D. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Albanesi, S. ;
Allocca, A. ;
Altin, P. A. ;
Amato, A. ;
Anand, C. ;
Anand, S. ;
Ananyeva, A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Andrade, T. ;
Andres, N. ;
Andric, T. ;
Angelova, S., V ;
Ansoldi, S. ;
Antelis, J. M. ;
Antier, S. ;
Appert, S. ;
Arai, K. ;
Araya, M. C. ;
Areeda, J. S. ;
Arene, M. ;
Arnaud, N. ;
Aronson, S. M. ;
Arun, K. G. ;
Asali, Y. ;
Ashton, G. ;
Assiduo, M. ;
Aston, S. M. ;
Astone, P. ;
Aubin, F. ;
Austin, C. ;
Babak, S. ;
Badaracco, F. .
PHYSICAL REVIEW D, 2024, 109 (02)
[6]   Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3 [J].
Abbott, R. ;
Abbott, T. D. ;
Acernese, F. ;
Ackley, K. ;
Adams, C. ;
Adhikari, N. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agarwal, D. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Akutsu, T. ;
de Alarcon, P. F. ;
Akcay, S. ;
Albanesi, S. ;
Allocca, A. ;
Altin, P. A. ;
Amato, A. ;
Anand, C. ;
Anand, S. ;
Ananyeva, A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Ando, M. ;
Andrade, T. ;
Andres, N. ;
Andric, T. ;
Angelova, S. V. ;
Ansoldi, S. ;
Antelis, J. M. ;
Antier, S. ;
Antonini, F. ;
Appert, S. ;
Arai, Koji ;
Arai, Koya ;
Arai, Y. ;
Araki, S. ;
Araya, A. ;
Araya, M. C. ;
Areeda, J. S. ;
Arene, M. ;
Aritomi, N. ;
Arnaud, N. ;
Arogeti, M. .
PHYSICAL REVIEW X, 2023, 13 (01)
[7]   Search for intermediate-mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo [J].
Abbott, R. ;
Abbott, T. D. ;
Acernese, F. ;
Ackley, K. ;
Adams, C. ;
Adhikari, N. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agarwal, D. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Akutsu, T. ;
Albanesi, S. ;
Allocca, A. ;
Altin, P. A. ;
Amato, A. ;
Anand, C. ;
Anand, S. ;
Ananyeva, A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Ando, M. ;
Andrade, T. ;
Andres, N. ;
Andric, T. ;
Angelova, S., V ;
Ansoldi, S. ;
Antelis, J. M. ;
Antier, S. ;
Appert, S. ;
Arai, K. ;
Arai, K. ;
Arai, Y. ;
Araki, S. ;
Araya, A. ;
Araya, M. C. ;
Areeda, J. S. ;
Arene, M. ;
Aritomi, N. ;
Arnaud, N. ;
Aronson, S. M. ;
Arun, K. G. ;
Asada, H. ;
Asali, Y. .
ASTRONOMY & ASTROPHYSICS, 2022, 659
[8]   Planck 2015 results XVII. Constraints on primordial non-Gaussianity [J].
Ade, P. A. R. ;
Aghanim, N. ;
Arnaud, M. ;
Arrojam, F. ;
Ashdown, M. ;
Aumont, J. ;
Baccigalupi, C. ;
Ballardini, M. ;
Banday, A. J. ;
Barreiro, R. B. ;
Bartolo, N. ;
Basak, S. ;
Battaner, E. ;
Benabed, K. ;
Benoit, A. ;
Benoit-Levy, A. ;
Bernard, J. -P. ;
Bersanelli, M. ;
Bielewicz, P. ;
Bock, J. J. ;
Bonaldi, A. ;
Bonavera, L. ;
Bond, J. R. ;
Borrill, J. ;
Bouchet, F. R. ;
Boulanger, F. ;
Bucher, M. ;
Burigana, C. ;
Butler, R. C. ;
Calabrese, E. ;
Cardoso, J. -F. ;
Catalano, A. ;
Challinor, A. ;
Chamballu, A. ;
Chiang, H. C. ;
Christensen, P. R. ;
Church, S. ;
Clements, D. L. ;
Colombi, S. ;
Colombo, L. P. L. ;
Combet, C. ;
Couchot, F. ;
Coulais, A. ;
Crill, B. P. ;
Curto, A. ;
Cuttaia, F. ;
Danese, L. ;
Davies, R. D. ;
Davis, R. J. ;
de Bernardis, P. .
ASTRONOMY & ASTROPHYSICS, 2016, 594
[9]   Intermediate and extreme mass-ratio inspirals - astrophysics, science applications and detection using LISA [J].
Amaro-Seoane, Pau ;
Gair, Jonathan R. ;
Freitag, Marc ;
Miller, M. Coleman ;
Mandel, Ilya ;
Cutler, Curt J. ;
Babak, Stanislav .
CLASSICAL AND QUANTUM GRAVITY, 2007, 24 (17) :R113-R169
[10]  
Amaro-Seoane P, 2017, Arxiv, DOI arXiv:1702.00786