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arXiv · 1803.04632

Growth of a Black Hole on a Self-Gravitating Radiation

Hyeong-Chan Kim
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Abstract

We feed a black hole on a self-gravitating radiation and observe what happens during the process. Considering a spherical shell of radiation, we show that the contribution of self-gravity makes the thermodynamic interaction through the bottom of the shell be distinguished from thermodynamic interaction through its top. The growth of a black hole horizon appears to be a sudden jump rather than a sequential increase. We additionally show that much of the entropy will be absorbed into the black hole only at the last moment of the collapse.

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Hyeong-Chan Kim. 2018-05-02. Growth of a Black Hole on a Self-Gravitating Radiation. https://doi.org/10.1140/epjc%2Fs10052-018-6487-4

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