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Black hole radiance, short distances and TeV gravity.
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| Agulló, Iván; Navarro Salas, José; Olmo Alba, Gonzalo | |||
| This document is a artículoDate2006 | |||
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Este documento está disponible también en : 10.1103/PhysRevLett.97.041302 |
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| 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 κlP<<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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22 - Física [1773]