Document Type
Conference Proceeding
Publication Date
1-1-2008
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 Klp << 1. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase. © 2008 World Scientific Publishing Co. Pte. Ltd.
Publication Source (Journal or Book title)
11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories - Proc. of the MG11 Meeting on General Relativity
First Page
1437
Last Page
1439
Recommended Citation
Agulló, I., Navarro-Salas, J., & Olmo, G. (2008). Short distances, black holes, and TeV gravity. 11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories - Proc. of the MG11 Meeting on General Relativity, 1437-1439. https://doi.org/10.1142/9789812834300_0166