title: Black hole radiance, short distances, and TeV gravity.
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 kappalp<<1. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.
authors.affiliation: Departamento de Física Teórica and IFIC, Centro Mixto Universidad de Valencia-CSIC, Universidad de Valencia, Burjassot-46100, Valencia, Spain. ivan.agullo@uv.es
authors.forename: Iván
authors.initials: I
authors.lastname: Agulló
authors.forename: José
authors.initials: J
authors.lastname: Navarro-Salas
authors.forename: Gonzalo J
authors.initials: GJ
authors.lastname: Olmo