Short distances, black holes, and TeV gravity

Details Short distances, black holes, and TeV gravity Short distances, black holes, and TeV gravity

2007-01-17

arxiv.org/abs/hep-th/0701162v1

Physics

High Energy Physics

High Energy Physics - Theory

4 pages. Contribution to the MG11 Meeting (Berlin, July 2006)

Scientific paper

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 $I^+$ to the Planckian spectrum. Thermality is preserved for black holes with $\kappa l_P << 1$. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.

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