Kiselev Black Holes in Anti-de Sitter Spacetime Are Not Viable

Fuente: arXiv
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Hauptverfasser: Xia, Jiayi, Ong, Yen Chin
Format: Preprint
Veröffentlicht: 2025
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author Xia, Jiayi
Ong, Yen Chin
author_facet Xia, Jiayi
Ong, Yen Chin
contents While the Kiselev black hole solution does not describe a perfect fluid quintessence, it is possible that dark energy fluid is not isotropic, and so one may hope that the solution may still describe at least locally a black hole embedded in such a dark energy fluid environment. Taking into account that the accelerated expansion of the Universe is caused by a dynamical dark energy fluid, and the actual underlying cosmological constant is negative as has been sometimes suggested, we show that the Kiselev solution is untenable as it is unstable against brane nucleation instability.
format Preprint
id arxiv_https___arxiv_org_abs_2512_01265
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Kiselev Black Holes in Anti-de Sitter Spacetime Are Not Viable
Xia, Jiayi
Ong, Yen Chin
General Relativity and Quantum Cosmology
High Energy Physics - Theory
While the Kiselev black hole solution does not describe a perfect fluid quintessence, it is possible that dark energy fluid is not isotropic, and so one may hope that the solution may still describe at least locally a black hole embedded in such a dark energy fluid environment. Taking into account that the accelerated expansion of the Universe is caused by a dynamical dark energy fluid, and the actual underlying cosmological constant is negative as has been sometimes suggested, we show that the Kiselev solution is untenable as it is unstable against brane nucleation instability.
title Kiselev Black Holes in Anti-de Sitter Spacetime Are Not Viable
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2512.01265