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arXiv · hep-th/0701162

Short distances, black holes, and TeV gravity

I. Agullo·J. Navarro-Salas·Gonzalo J. Olmo
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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 $I^+$ 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.

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I. Agullo, J. Navarro-Salas, Gonzalo J. Olmo. 2007-01-17. Short distances, black holes, and TeV gravity. https://doi.org/10.1142/9789812834300_0166

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