Finite-mass correction to 2D Black-hole evaporation rate
General Relativity and Quantum Cosmology
2013-05-30 v2 High Energy Physics - Theory
Abstract
We numerically analyze the evolution of a two-dimensional dilatonic black hole, within the CGHS model. We focus our attention on the finite-mass corrections to the universal evaporation rate which applies at the large-mass limit. Our numerical results confirm a previous theoretical prediction for the first-order () correction. In addition, our results strongly suggest that the next-order () term vanishes, and provide a rough estimate for the third-order term.
Keywords
Cite
@article{arxiv.1201.6386,
title = {Finite-mass correction to 2D Black-hole evaporation rate},
author = {Liora Dori and Amos Ori},
journal= {arXiv preprint arXiv:1201.6386},
year = {2013}
}
Comments
12 pages. Typos corrected; Few minor corrections to match the published version; Note added in proof