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2016

Black hole evaporation in conformal gravity

Bambi, Cosimo, Modesto, Leonardo, Porey, Shiladitya et al.

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We study the formation and the evaporation of a spherically symmetric black hole in conformal gravity.

From the collapse of a spherically symmetric thin shell of radiation, we find a singularity-free non-rotating black hole.
This black hole has the same Hawking temperature as a Schwarzschild black hole with the same mass, and it completely evaporates either in a finite or in an infinite time, depending on the ensemble.
We consider the analysis both in the canonical and in the micro-canonical statistical ensembles.

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