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Hawking Radiation as Tunnelling in Static Black Holes

Wenbiao Liu
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Abstract

Hawking radiation can usefully be viewed as a semi-classical tunnelling process that originates at the black hole horizon. The conservation of energy implies the effect of self-gravitation. For a static black hole, a generalized Painleve coordinate system is introduced, and Hawking radiation as tunnelling under the effect of self-gravitation is investigated. The corrected radiation is consistent with the underlying unitary theory.

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Wenbiao Liu. 2005-12-16. Hawking Radiation as Tunnelling in Static Black Holes. https://arxiv.org/abs/gr-qc/0512098

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