Hawking Radiation of Dirac Particles in a Variable-mass Kerr Space-time

Preprint

18 April 2001

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/0104055

Abstract

Hawking effect of Dirac particles in a variable-mass Kerr space-time is investigated by using a method called as the generalized tortoise coordinate transformation. The location and the temperature of the event horizon of the non-stationary Kerr black hole are derived. It is shown that the temperature and the shape of the event horizon depend not only on the time but also on the angle. However, the Fermi-Dirac spectrum displays a residual term which is absent from that of Bose-Einstein distribution.

Keywords

COORDINATE TRANSFORMATION
VARIABLE MASS KERR
DIRAC PARTICLES
KERR SPACE
BLACK HOLE
HAWKING

All Related Versions

Version 1, 2001-04-18, ArXiv
Published version: General Relativity and Gravitation, 33 (7), 1181.

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