Subtleties in the quasi-classical calculation of Hawking radiation

Details Subtleties in the quasi-classical calculation of Hawking radiation Subtleties in the quasi-classical calculation of Hawking radiation

2008-05-17

arxiv.org/abs/0805.2653v2

Int.J.Mod.Phys.D17:2453-2458,2008

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages revtex. Honorable Mention in 2008 GRF essay contest, typos fixed, sign errors corrected. To be published in Special Is

Scientific paper

10.1142/S0218271808013947

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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