Hawking Radiation of Dirac Particles in an Arbitrarily Accelerating Kinnersley Black Hole
General Relativity and Quantum Cosmology
2021-10-20 v1
Abstract
Quantum thermal effect of Dirac particles in an arbitrarily accelerating Kinnersley black hole is investigated by using the method of generalized tortoise coordinate transformation. Both the location and the temperature of the event horizon depend on the advanced time and the angles. The Hawking thermal radiation spectrum of Dirac particles contains a new term which represents the interaction between particles with spin and black holes with acceleration. This spin-acceleration coupling effect is absent from the thermal radiation spectrum of scalar particles.
Keywords
Cite
@article{arxiv.gr-qc/0202070,
title = {Hawking Radiation of Dirac Particles in an Arbitrarily Accelerating Kinnersley Black Hole},
author = {S. Q. Wu and X. Cai},
journal= {arXiv preprint arXiv:gr-qc/0202070},
year = {2021}
}
Comments
Revtex, 12pt, 16 pages, no figure, to appear in Gen. Rel. Grav. 34 (2002) N0. 8