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Primordial Black Holes as a dark matter candidate

Green, Anne M.; Kavanagh, Bradley J.

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ANNE GREEN anne.green@nottingham.ac.uk
Professor of Physics

Bradley J. Kavanagh



Abstract

The detection of gravitational waves from mergers of tens of Solar mass black hole binaries has led to a surge in interest in Primordial Black Holes (PBHs) as a dark matter candidate. We aim to provide a (relatively) concise overview of the status of PBHs as a dark matter candidate, circa Summer 2020. First we review the formation of PBHs in the early Universe, focusing mainly on PBHs formed via the collapse of large density perturbations generated by inflation. Then we review the various current and future constraints on the present day abundance of PBHs. We conclude with a discussion of the key open questions in this field.

Journal Article Type Article
Acceptance Date Oct 14, 2020
Online Publication Date Oct 27, 2020
Publication Date Feb 10, 2021
Deposit Date Oct 23, 2020
Publicly Available Date Oct 28, 2021
Journal Journal of Physics G: Nuclear and Particle Physics
Print ISSN 0954-3899
Electronic ISSN 1361-6471
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 48
Issue 4
Article Number 043001
DOI https://doi.org/10.1088/1361-6471/abc534
Keywords Nuclear and High Energy Physics
Public URL https://nottingham-repository.worktribe.com/output/4985473
Publisher URL https://iopscience.iop.org/article/10.1088/1361-6471/abc534

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