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Spinning primordial black holes formed during a matter-dominated era

Abstract:
This review is an up-to-date account of the use of numerical relativity to study dynamical, strong-gravity environments in a cosmological context. First, we provide a gentle introduction into the use of numerical relativity in solving cosmological spacetimes, aimed at both cosmologists and numerical relativists. Second, we survey the present body of work, focusing on general relativistic simulations, organised according to the cosmological history—from cosmogenesis, through the early hot Big Bang, to the late-time evolution of the universe. We discuss the present state-of-the-art, and suggest directions in which future work can be fruitfully pursued
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1475-7516/2023/10/067

Authors

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Role:
Author
ORCID:
0000-0002-4505-0808
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-9584-5791
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Role:
Author
ORCID:
0000-0002-6227-9540


Publisher:
IOP Publishing
Journal:
Journal of Cosmology and Astroparticle Physics More from this journal
Volume:
2023
Issue:
10
Pages:
067-067
Publication date:
2023-10-26
DOI:
ISSN:
1475-7508


Language:
English
Keywords:
Pubs id:
1575241
Local pid:
pubs:1575241
Source identifiers:
W4387955784
Deposit date:
2026-06-04
ARK identifier:
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