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Cited by 497

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Inflation and primordial black holes as dark matter

Ivanov, P., Naselsky, P., Novikov, I.·1994·Physical Review D

Abstract

We discuss the hypothesis that a large (or even a major) fraction of dark matter in the Universe consists of primordial black holes (PBH's). PBH's may arise from adiabatic quantum fluctuations appearing during inflation. We demonstrate that the inflation potential V(cphi) leading to the formation of a great number of PBH's should have a feature of the ``plateau''-type in some range ${\mathit{cphi}}_{1}$cphi${\mathit{cphi}}_{2}$ of the inflation field cphi. The mass spectrum of PBH's for such a potential is calculated.

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Cites

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Research works printed but not linked: 39

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Metadata

Authors
Ivanov, P., Naselsky, P., & Novikov, I.
Venue
Physical Review D
Published
1994-12-15
Volume
50
Issue
12
Pages
7173-7178
ISSN
0556-2821 (ISSN-L)
OpenAlex
W2141106168
Cited by
497
References
3
FWCI
3.44
Type
journal article
Language
en
Open access
closed

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Ivanov, P., Naselsky, P., & Novikov, I. (1994). Inflation and primordial black holes as dark matter. Physical Review D. https://doi.org/10.1103/physrevd.50.7173

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