Hawking Radiation from Fluctuating Black Holes
General Relativity and Quantum Cosmology
2014-11-20 v1 High Energy Physics - Theory
Abstract
Classically, black Holes have the rigid event horizon. However, quantum mechanically, the event horizon of black holes becomes fuzzy due to quantum fluctuations. We study Hawking radiation of a real scalar field from a fluctuating black hole. To quantize metric perturbations, we derive the quadratic action for those in the black hole background. Then, we calculate the cubic interaction terms in the action for the scalar field. Using these results, we obtain the spectrum of Hawking radiation in the presence of interaction between the scalar field and the metric. It turns out that the spectrum deviates from the Planck spectrum due to quantum fluctuations of the metric.
Cite
@article{arxiv.1005.0286,
title = {Hawking Radiation from Fluctuating Black Holes},
author = {Tomohiro Takahashi and Jiro Soda},
journal= {arXiv preprint arXiv:1005.0286},
year = {2014}
}
Comments
35pages, 4 figures