Subtleties in the quasi-classical calculation of Hawking radiation
classification
🌀 gr-qc
hep-th
keywords
contributionhawkingactioncomingpartquasi-classicalradiationtemperature
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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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