Evaporating black holes in de Sitter expanding universe

Fuente: arXiv
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Autore principale: Cotaescu, Ion I.
Natura: Preprint
Pubblicazione: 2024
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author Cotaescu, Ion I.
author_facet Cotaescu, Ion I.
contents Models of evaporating black holes are constructed using the new solutions of Einstein's equations with perfect fluid in space-times with FLRW asymptotic behaviour derived recently [I. I. Cotaescu, Eur. Phys. J. C (2022) 82:86]. The dynamics of these models is exclusively due to the interplay between black holes and their environments, without resorting to additional matter sources or thermodynamic considerations. During evaporation the black hole mass dissipates into a cloud of dust which replaces the black hole while the background expands tending to the asymptotic one.
format Preprint
id arxiv_https___arxiv_org_abs_2411_15258
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Evaporating black holes in de Sitter expanding universe
Cotaescu, Ion I.
General Relativity and Quantum Cosmology
Models of evaporating black holes are constructed using the new solutions of Einstein's equations with perfect fluid in space-times with FLRW asymptotic behaviour derived recently [I. I. Cotaescu, Eur. Phys. J. C (2022) 82:86]. The dynamics of these models is exclusively due to the interplay between black holes and their environments, without resorting to additional matter sources or thermodynamic considerations. During evaporation the black hole mass dissipates into a cloud of dust which replaces the black hole while the background expands tending to the asymptotic one.
title Evaporating black holes in de Sitter expanding universe
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2411.15258