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2016

The fate of Schwarzschild-de Sitter Black Holes in $f(R)$ gravity

Addazi, Andrea, Capozziello, Salvatore

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The semiclassical effects of antievaporating black holes can be discussed in the framework of $f(R)$ gravity.

In particular, the Bousso-Hawking-Nojiri-Odinstov antievaporation instability of degenerate Schwarzschild-de Sitter black holes (the so called Nariai space-time) leads to a dynamical increasing of black hole horizon in $f(R)$ gravity.
This phenomenon causes the following transition: emitting marginally trapped surfaces become space-like surfaces before the effective Bekenstein-Hawking emission time.
As a consequence, Bousso-Hawking thermal radiation cannot be emitted in an antievaporating Nariai black hole.

The fate of Schwarzschild-de Sitter Black Holes in $f(R)$ gravity · Around

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