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Anti-Evaporation of Bardeen de-Sitter Black Holes

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arxiv 1704.01831 v2 pith:CCI4K7W2 submitted 2017-03-30 physics.gen-ph

Dharm Veer Singh , Naveen K. Singh This is my paper · ORCID
classification physics.gen-ph
keywords blackanti-evaporationbardeende-sitterholeholeshorizonnariai
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In this paper, we discuss the possibility of the anti-evaporation of degenerate Bardeen de-Sitter black hole. We solve the perturbation equations around the Nariai space-time. The solution of one of the perturbations related to the horizon size demonstrates that horizon of such black hole is constant. The other perturbation is also found to be stable. We further study thermodynamical properties of such black holes. We observe double phase transition at the Nariai limit.

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  1. (Anti-)evaporation of Schwarzschild-de Sitter black holes revisited

    gr-qc 2019-08 conditional novelty 6.0 of 10

    Within the Bousso-Hawking effective action, the Schwarzschild-de Sitter asymptotic is excluded, which undermines earlier anti-evaporation results that used the Nariai limit.

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