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Hawking Radiation as Tunneling in Static Black Holes

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Hawking radiation can usefully be viewed as a semi-classical tunneling 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 Painlevé coordinate system is introduced, and Hawking radiation as tunneling under the effect of self-gravitation is investigated. The corrected radiation is consistent with the underlying unitary theory.

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