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Paper detail

Short distances, black holes, and TeV gravity

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 $κl_P << 1$. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.

preprint2007arXivOpen access
I. AgulloJ. Navarro-SalasGonzalo J. Olmo
hep-th
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I. AgulloJ. Navarro-SalasGonzalo J. Olmo

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