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Black Hole Production of Monopoles in the Early Universe

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arxiv 2109.00039 v1 pith:UULFT3GU submitted 2021-08-31 hep-ph

classification hep-ph
keywords blackuniverseholeholesmonopolesearlyevaporatingplasma
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abstract

In the early universe, evaporating black holes heat up the surrounding plasma and create a temperature profile around the black hole that can be more important than the black hole itself. As an example, we demonstrate how the hot plasma surrounding evaporating black holes can efficiently produce monopoles via the Kibble-Zurek mechanism. In the case where black holes reheat the universe, reheat temperatures above $\sim 500$ GeV can already lead to monopoles overclosing the universe.

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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. Monopole Catalyzed Baryogenesis with a $\theta$ angle

    hep-ph 2024-12 reject novelty 7.0 of 10

    Claims that Callan-Rubakov monopole catalysis biased by a tiny theta-term can generate the observed baryon asymmetry at T~100 GeV with monopole densities below current bounds.

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