Short distances, black holes, and TeV gravity
High Energy Physics - Theory
2016-11-15 v1
Abstract
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes it possible to estimate, within the conventional semiclassical theory, the contribution of ultrashort distances at to the Planckian spectrum. Thermality is preserved for black holes with . However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.
Cite
@article{arxiv.hep-th/0701162,
title = {Short distances, black holes, and TeV gravity},
author = {I. Agullo and J. Navarro-Salas and Gonzalo J. Olmo},
journal= {arXiv preprint arXiv:hep-th/0701162},
year = {2016}
}
Comments
4 pages. Contribution to the MG11 Meeting (Berlin, July 2006)