Primordial Black Holes from Supersymmetry in the Early Universe

Cotner, Eric; Kusenko, Alexander

doi:10.1103/PhysRevLett.119.031103

Title: Primordial Black Holes from Supersymmetry in the Early Universe

Journal Article · Fri Jul 21 00:00:00 EDT 2017 · Physical Review Letters

DOI:https://doi.org/10.1103/PhysRevLett.119.031103· OSTI ID:1609065

Cotner, Eric ^[1]; Kusenko, Alexander ^[2]

Univ. of California, Los Angeles, CA (United States)
Univ. of California, Los Angeles, CA (United States); Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)

Supersymmetric extensions of the standard model generically suggest that in the early universe a scalar condensate can form and fragment into Q-balls before decaying. If the Q-balls dominate the energy density for some period of time, the relatively large fluctuations in their number density can lead to formation of primordial black holes (PBH). Other scalar fields, unrelated to supersymmetry, can play a similar role. For a general charged scalar field, this robust mechanism can generate black holes over the entire mass range allowed by observational constraints, with a sufficient abundance to account for all dark matter in some parameter ranges. In the case of supersymmetry the mass range is limited from above by 10²³g. We further comment on the role that topological defects can play for PBH formation in a similar fashion.

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Research Organization:: Univ. of California, Los Angeles, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: SC0009937

OSTI ID:: 1609065

Alternate ID(s):: OSTI ID: 1372417

Journal Information:: Physical Review Letters, Vol. 119, Issue 3; ISSN 0031-9007

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 85 works

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Propagation of self-localized $Q$ -ball solitons in the ${}^{3}{He}$ universe Autti, S.; Heikkinen, P. J.; Volovik, G. E. Physical Review B, Vol. 97, Issue 1 https://doi.org/10.1103/physrevb.97.014518	journal	January 2018
Analytic description of primordial black hole formation from scalar field fragmentation Cotner, Eric; Kusenko, Alexander; Sasaki, Misao Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 10 https://doi.org/10.1088/1475-7516/2019/10/077	journal	October 2019
Gravitational wave signatures of inflationary models from Primordial Black Hole dark matter García-Bellido, Juan; Peloso, Marco; Unal, Caner Journal of Cosmology and Astroparticle Physics, Vol. 2017, Issue 09 https://doi.org/10.1088/1475-7516/2017/09/013	journal	September 2017
Primordial black holes from inflaton and spectator field perturbations in a matter-dominated era Carr, Bernard; Tenkanen, Tommi; Vaskonen, Ville Physical Review D, Vol. 96, Issue 6 https://doi.org/10.1103/physrevd.96.063507	journal	September 2017
A Preferred Mass Range for Primordial Black Hole Formation and Black Holes as Dark Matter Revisited Georg, Julian; Watson, Scott arXiv https://doi.org/10.48550/arxiv.1703.04825	text	January 2017
Effect of Inhomogeneity on Primordial Black Hole Formation in the Matter Dominated Era Kokubu, Takafumi; Kyutoku, Koutarou; Kohri, Kazunori arXiv https://doi.org/10.48550/arxiv.1810.03490	text	January 2018
Analytic Description of Primordial Black Hole Formation from Scalar Field Fragmentation Cotner, Eric; Kusenko, Alexander; Sasaki, Misao arXiv https://doi.org/10.48550/arxiv.1907.10613	text	January 2019

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