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Subtleties in the quasi-classical calculation of Hawking radiation
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Subtleties in the quasi-classical calculation of Hawking radiation
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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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Cited by 1 Pith paper
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Thermal bath induced suppression of Hawking radiation
A Schwarzschild black hole coupled bilinearly to an environmental scalar field radiates less than Hawking's prediction, according to a semiclassical Keldysh calculation.
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