Estimating Hawking radiation for exotic black holes
General Relativity and Quantum Cosmology
2009-10-31 v2
Abstract
We study about an approximation method of the Hawking radiation. We analyze an massless scalar field in exotic black hole backgrounds models which have peculiar properties in black hole thermodynamics (monopole black hole in SO(3) Einstein-Yang-Mills-Higgs system and dilatoic black hole in Einstein-Maxwell-dilaton system). A scalar field is assumed not to be couple to matter fields consisting of a black hole background. Except for extreme black holes, we can well approximate the Hawking radiaition by `black body' one with Hawking temperature estimated at a radius of a critical impact parameter.
Keywords
Cite
@article{arxiv.gr-qc/0005093,
title = {Estimating Hawking radiation for exotic black holes},
author = {Takashi Tamaki and Kei-ichi Maeda},
journal= {arXiv preprint arXiv:gr-qc/0005093},
year = {2009}
}
Comments
4 pages, 7 figures