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Compact extra dimensions as the source of primordial black holes

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arxiv 2204.06360 v1 pith:BBHSPXRP submitted 2022-04-13 gr-qc

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keywords blackholescompactdimensionsextrainflationmodelprimordial
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abstract

We discuss the model of the primordial black holes formation at the reheating stage. These small massive black holes appear due to specific properties of the compact extra dimensions. The latter gives rise the low energy model containing the effective scalar field potential capable for the domain walls production. Formed during inflation, these walls are quite dense so they collapse soon after inflation ends. The discussion is performed within the scope of multidimensional $f(R)$-gravity.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Four years of wide-field search for nanosecond optical transients with the TAIGA-HiSCORE Cherenkov array

    astro-ph.IM 2024-11 conditional novelty 5.0 of 10

    Four seasons of TAIGA-HiSCORE data show no nanosecond optical transients, setting an upper limit of about 1e-3 events per steradian per hour.

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