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Anti-Evaporation of Schwarzschild-de Sitter Black Holes in $F(R)$ gravity
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abstract
We studied the anti-evaporation of degenerate Schwarzschild-de Sitter black hole (so-called Nariai space-time) in modified $F(R)$ gravity. The analysis of perturbations of the Nariai black hole is done with the conclusion that anti-evaporation may occur in such a theory already on classical level. For several power-law $F(R)$ gravities which may describe the inflation and/or dark energy eras we presented the theory parameters bounds for occurrence of anti-evaporation and conjectured creation of infinite number of horizons.
Forward citations
Cited by 2 Pith papers
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The Fate of Nucleated Black Holes in de Sitter Quantum Gravity
Nucleated maximal-mass black holes in de Sitter space undergo thermal Hawking evaporation in smooth quantum states and return fully to the empty de Sitter vacuum.
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(Anti-)evaporation of Schwarzschild-de Sitter black holes revisited
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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