Black hole radiance, short distances, and TeV gravity

Details Black hole radiance, short distances, and TeV gravity Black hole radiance, short distances, and TeV gravity

2006-04-06

arxiv.org/abs/hep-th/0604044v2

Phys.Rev.Lett. 97 (2006) 041302

Physics

High Energy Physics

High Energy Physics - Theory

LaTeX, 4 pages, 1 figure. Misprints corrected

Scientific paper

10.1103/PhysRevLett.97.041302

Using a derivation of black hole radiance in terms of two-point functions one
can provide a quantitative estimate of the contribution of short distances to
the 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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