Evaporation of Primordial Charged Black Holes: Timescale and Evolution of Thermodynamic Parameters
Autor: | José Antonio de Freitas Pacheco |
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Jazyk: | angličtina |
Rok vydání: | 2024 |
Předmět: | |
Zdroj: | Symmetry, Vol 16, Iss 7, p 895 (2024) |
Druh dokumentu: | article |
ISSN: | 16070895 2073-8994 |
DOI: | 10.3390/sym16070895 |
Popis: | The evolution of primordial black holes formed during the reheating phase is revisited. For reheating temperatures in the range of 1012–1013 GeV, the initial masses are respectively of the order of 1010–108MP, where MP is the Planck mass. These newborn black holes have a small charge-to-mass ratio of the order of 10−3, a consequence of statistical fluctuations present in the plasma constituting the collapsing matter. Charged black holes can be rapidly discharged by the Schwinger mechanism, but one expects that, for very light black holes satisfying the condition M/MP< |
Databáze: | Directory of Open Access Journals |
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