Black Hole Radiance, Short Distances, and TeV Gravity

Iván Agulló, José Navarro-Salas, and Gonzalo J. Olmo
Phys. Rev. Lett. 97, 041302 – Published 26 July 2006

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 κlP1. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.

  • Figure
  • Received 10 April 2006

DOI:https://doi.org/10.1103/PhysRevLett.97.041302

©2006 American Physical Society

Authors & Affiliations

Iván Agulló1,*, José Navarro-Salas1,†, and Gonzalo J. Olmo2,‡

  • 1Departamento de Física Teórica and IFIC, Centro Mixto Universidad de Valencia-CSIC, Universidad de Valencia, Burjassot-46100, Valencia, Spain
  • 2Physics Department, University of Wisconsin-Milwaukee, P.O. Box 413, Milwaukee, Wisconsin 53201 USA

  • *Electronic address: ivan.agullo@uv.es
  • Electronic address: jnavarro@ific.uv.es
  • Electronic address: olmoalba@uwm.edu

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Issue

Vol. 97, Iss. 4 — 28 July 2006

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