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Radiation Ball as a Black Hole

Yukinori Nagatani
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Abstract

A structure of the radiation-ball which is identified as a Schwarzschild black hole is found out by investigating the backreaction of Hawking radiation into space-time. The structure consists of the radiation which is gravitationally bounded in the ball and of a singularity. The entropy of the radiation in the ball is proportional to the surface-area of the ball and nearly equals to the Bekenstein entropy. The Hawking radiation is regarded as a leak-out from the ball. There arises no information paradox because there exists no horizon in the structure.

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Yukinori Nagatani. 2003-12-07. Radiation Ball as a Black Hole. https://arxiv.org/abs/hep-th/0310185

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