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arXiv · 0805.2653

Subtleties in the quasi-classical calculation of Hawking radiation

Emil T. Akhmedov·Terry Pilling·Douglas Singleton
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Abstract

he quasi-classical method of deriving Hawking radiation is investigated. In order to recover the original Hawking temperature one must take into account a previously ignored contribution coming from the temporal part of the action. This contribution plus a contribution coming from the spatial part of the action gives the correct temperature.

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Emil T. Akhmedov, Terry Pilling, Douglas Singleton. 2008-10-02. Subtleties in the quasi-classical calculation of Hawking radiation. https://doi.org/10.1142/s0218271808013947

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