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Hawking temperature and higher order calculations · Around

2009

Hawking temperature and higher order calculations

Chatterjee, Bhramar, Mitra, P.

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Hawking radiation has recently been explained by using solutions of wave equations across black hole horizons in a WKB approximation.

Higher order calculations using both usual and non-singular coordinates are found to change the solution for zero spin, but this change is not an alteration of the Hawking temperature.
For spin 1/2, there is no correction to the simplest form of the solution.

Built on

D. Brill and J. Wheeler, Rev. Mod. Phys. 29
Original
1957
Earlier work this paper cites.
S. W. Hawking, Comm. Math. Phys. 43
1975
Earlier work this paper cites.
J. B. Hartle and S. W. Hawking, Phys. Rev. D13
1976
Earlier work this paper cites.
K. Srinivasan and T. Padmanabhan, Phys. Rev. D60
1999
Earlier work this paper cites.

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Then

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Later among the works it cites.
R. Kerner and R. B. Mann, Phys. Rev. D75
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2008
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R. Banerjee and B. R. Majhi, JHEP 0806
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Later among the works it cites.

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