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arXiv · 1302.4733

A Self-consistent Model of the Black Hole Evaporation

Hikaru Kawai·Yoshinori Matsuo·Yuki Yokokura
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Abstract

We construct a self-consistent model which describes a black hole from formation to evaporation including the back reaction from the Hawking radiation. In the case where a null shell collapses, at the beginning the evaporation occurs, but it stops eventually, and a horizon and singularity appear. On the other hand, in the generic collapse process of a continuously distributed null matter, the black hole evaporates completely without forming a macroscopically large horizon nor singularity. We also find a stationary solution in the heat bath, which can be regarded as a normal thermodynamic object.

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Hikaru Kawai, Yoshinori Matsuo, Yuki Yokokura. 2013-02-19. A Self-consistent Model of the Black Hole Evaporation. https://doi.org/10.1142/s0217751x13500504

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