Hawking Radiation of Dirac Particles in a Variable-mass Kerr Space-time
General Relativity and Quantum Cosmology
2015-06-25 v1
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
Cite
@article{arxiv.gr-qc/0104055,
title = {Hawking Radiation of Dirac Particles in a Variable-mass Kerr Space-time},
author = {S. Q. Wu and X. Cai},
journal= {arXiv preprint arXiv:gr-qc/0104055},
year = {2015}
}
Comments
12 pages in 12pt Revtex, no figure, to appear in Gen. Rel. Grav. Vol.33, No.7 (2001)