2000 character limit reached
Spinning primordial black holes formed during a matter-dominated era (2306.11810v2)
Published 20 Jun 2023 in astro-ph.CO and gr-qc
Abstract: We study the formation of spinning primordial black holes during an early matter-dominated era. Using non-linear 3+1D general relativistic simulations, we compute the efficiency of mass and angular momentum transfer in the process -- which we find to be $\mathcal{O}(10\%)$ and $\mathcal{O}(5\%)$, respectively. We show that subsequent evolution is important due to the seed PBH accreting non-rotating matter from the background, which decreases the dimensionless spin. Unless the matter era is short, we argue that the final dimensionless spin will be negligible.
- B. J. Carr and S. W. Hawking, Monthly Notices of the Royal Astronomical Society 168, 399 (1974), https://academic.oup.com/mnras/article-pdf/168/2/399/8079885/mnras168-0399.pdf .
- S. Hawking, Monthly Notices of the Royal Astronomical Society 152, 75 (1971), https://academic.oup.com/mnras/article-pdf/152/1/75/9360899/mnras152-0075.pdf .
- Y. B. Zel’dovich and I. D. Novikov, Soviet Astronomy 10, 602 (1967).
- B. Carr and F. Kuhnel, Ann. Rev. Nucl. Part. Sci. 70, 355 (2020), arXiv:2006.02838 [astro-ph.CO] .
- D. N. Page and S. W. Hawking, Astrophys. J. 206, 1 (1976).
- B. J. Carr, Astrophys. J. 206, 8 (1976).
- E. L. Wright, Astrophys. J. 459, 487 (1996), arXiv:astro-ph/9509074 .
- J. H. MacGibbon and B. J. Carr, Astrophys. J. 371, 447 (1991).
- B. J. Carr and M. J. Rees, Monthly Notices of the Royal Astronomical Society 206, 801 (1984), https://academic.oup.com/mnras/article-pdf/206/4/801/2902772/mnras206-0801.pdf .
- R. Bean and J. a. Magueijo, Phys. Rev. D 66, 063505 (2002).
- M. R. S. Hawkins, Nature (London) 366, 242 (1993).
- Hawkins, M. R. S., A&A 633, A107 (2020).
- R. Abbott et al. (LIGO Scientific, Virgo), Astrophys. J. Lett. 900, L13 (2020), arXiv:2009.01190 [astro-ph.HE] .
- V. Vaskonen and H. Veermäe, Phys. Rev. Lett. 126, 051303 (2021), arXiv:2009.07832 [astro-ph.CO] .
- K. Kohri and T. Terada, Phys. Lett. B 813, 136040 (2021), arXiv:2009.11853 [astro-ph.CO] .
- G. Domènech and S. Pi, Sci. China Phys. Mech. Astron. 65, 230411 (2022), arXiv:2010.03976 [astro-ph.CO] .
- B. J. Carr, Astrophys. J. 201, 1 (1975).
- G. V. Bicknell and R. N. Henriksen, Astrophys. J. 232, 670 (1979).
- M. W. Choptuik, Phys. Rev. Lett. 70, 9 (1993).
- C. R. Evans and J. S. Coleman, Phys. Rev. Lett. 72, 1782 (1994).
- J. C. Niemeyer and K. Jedamzik, Physical Review Letters 80, 5481–5484 (1998).
- A. M. Green and A. R. Liddle, Physical Review D 60 (1999), 10.1103/physrevd.60.063509.
- I. Musco and J. C. Miller, Class. Quant. Grav. 30, 145009 (2013), arXiv:1201.2379 [gr-qc] .
- B. J. Carr and J. E. Lidsey, Phys. Rev. D 48, 543 (1993).
- H. M. Hodges and G. R. Blumenthal, Phys. Rev. D 42, 3329 (1990).
- A. Taruya, Physical Review D 59 (1999), 10.1103/physrevd.59.103505.
- B. A. Bassett and S. Tsujikawa, Physical Review D 63 (2001), 10.1103/physrevd.63.123503.
- S. Clesse and J. García-Bellido, Physical Review D 92 (2015), 10.1103/physrevd.92.023524.
- J. García-Bellido and E. Ruiz Morales, Physics of the Dark Universe 18, 47–54 (2017).
- M. Crawford and D. N. Schramm, Nature 298, 538 (1982).
- I. G. Moss, Phys. Rev. D 50, 676 (1994).
- N. Kitajima and F. Takahashi, JCAP 11, 060 (2020), arXiv:2006.13137 [hep-ph] .
- K. Kawana and K.-P. Xie, Phys. Lett. B 824, 136791 (2022), arXiv:2106.00111 [astro-ph.CO] .
- T. H. Jung and T. Okui, (2021), arXiv:2110.04271 [hep-ph] .
- C. J. Hogan, Phys. Lett. 143B, 87 (1984).
- S. Hawking, Phys. Lett. B 231, 237 (1989).
- A. Polnarev and R. Zembowicz, Phys. Rev. D 43, 1106 (1991).
- J. Garriga and M. Sakellariadou, Phys. Rev. D48, 2502 (1993), arXiv:hep-th/9303024 .
- R. Caldwell and P. Casper, Phys. Rev. D53, 3002 (1996), arXiv:gr-qc/9509012 .
- G. Bertone et al., SciPost Phys. Core 3, 007 (2020), arXiv:1907.10610 [astro-ph.CO] .
- S. M. Carroll and M. Kaplinghat, Phys. Rev. D 65, 063507 (2002), arXiv:astro-ph/0108002 .
- D. Hooper and H. Xiao, (2023), arXiv:2306.07339 [hep-ph] .
- M. Khlopov and A. Polnarev, Phys. Lett. B97, 383 (1980).
- A. G. Polnarev and M. Y. Khlopov, Soviet Astronomy 26, 9 (1982).
- F. Kuhnel, Eur. Phys. J. C 80, 243 (2020), arXiv:1909.04742 [astro-ph.CO] .
- S. Chongchitnan and J. Silk, Phys. Rev. D 104, 083018 (2021), arXiv:2109.12268 [astro-ph.CO] .
- M. He and T. Suyama, Phys. Rev. D 100, 063520 (2019), arXiv:1906.10987 [astro-ph.CO] .
- A. M. Green and A. R. Liddle, Phys. Rev. D 56, 6166 (1997).
- E. Cotner and A. Kusenko, Phys. Rev. Lett. 119, 031103 (2017), arXiv:1612.02529 [astro-ph.CO] .
- J. Georg and S. Watson, JHEP 09, 138 (2017), arXiv:1703.04825 [astro-ph.CO] .
- GRChombo, “Spinning primordial black holes formed during a matter-dominated era,” (2023), https://youtu.be/CC4xBLol4aE.
- A. Einstein, Annalen der Physik 354, 769 (1916).
- J. Thornburg, Class. Quant. Grav. 21, 743 (2004), arXiv:gr-qc/0306056 .
- T. W. Baumgarte and S. L. Shapiro, Numerical Relativity: Solving Einstein’s Equation on the Computer (Cambridge University Press, 2010).
- G. C. McVittie, Mon. Not. Roy. Astron. Soc. 93, 325 (1933).
Sponsor
Paper Prompts
Sign up for free to create and run prompts on this paper using GPT-5.
Top Community Prompts
Collections
Sign up for free to add this paper to one or more collections.