Abstract
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 . However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.
- Received 10 April 2006
DOI:https://doi.org/10.1103/PhysRevLett.97.041302
©2006 American Physical Society