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  Motion of Primordial Black Holes in the Early Universe and Their Likely Distribution Today

Islam, J. N., & Schutz, B. F. (1980). Motion of Primordial Black Holes in the Early Universe and Their Likely Distribution Today. General Relativity and Gravitation, 12(11), 881-893. doi:10.1007/BF00757357.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-7554-8 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-7557-2
Genre: Journal Article

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 Creators:
Islam, Jamal N.1, Author
Schutz, Bernard F.1, 2, Author           
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1External Organizations, Department of Applied Mathematics and Astronomy, University College, Cardiff, Wales, ou_persistent22              
2Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              

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 Abstract: We look in detail at those effects which slow down black holes of mass sim1015 g and affect their spatial distribution today. In particular we treat effects caused by the charge fluctuations of the hole which result from quantum-mechanical processes. The dominant energyloss mechanism for the holes is the expansion of the universe, which leaves them virtually at rest at the time of galaxy formation. The resultant violent relaxation should concentrate roughly half of them in present-day galaxies and their halos.

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 Dates: 1980-11
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: DOI: 10.1007/BF00757357
eDoc: 60594
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Title: General Relativity and Gravitation
Source Genre: Journal
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Pages: - Volume / Issue: 12 (11) Sequence Number: - Start / End Page: 881 - 893 Identifier: ISSN: 1572-9532