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Hawking radiation as tunneling for extremal and rotating black holes

Marco Angheben1, Mario Nadalini1,2, Luciano Vanzo1,2 and Sergio Zerbini1,2

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The issue concerning semi-classical methods recently developed in deriving the conditions for Hawking radiation as tunneling, is revisited and applied also to rotating black hole solutions as well as to the extremal cases. It is noticed how the tunneling method fixes the temperature of extremal black hole to be zero, unlike the euclidean regularity method that allows an arbitrary compactification period. A comparison with other approaches is presented.

Keywords

Black Holes

Space-Time Symmetries

 

E-print Number: hep-th/0503081

Cited: by |

Refers: to

PACS

04.70.-s Physics of black holes

11.10.-z Field theory

Subjects

Gravitation and cosmology

Particle physics and field theory

Dates

Issue 05 (May 2005)

Received 14 March 2005, accepted for publication 9 April 2005

Published 5 May 2005



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