Black Holes at Future Colliders and in Cosmic Rays

Details Black Holes at Future Colliders and in Cosmic Rays Black Holes at Future Colliders and in Cosmic Rays

2003-10-16

arxiv.org/abs/hep-ex/0310034v1

Eur.Phys.J.C33:s927-s931,2004

Physics

High Energy Physics

High Energy Physics - Experiment

To appear in Proc. International Europhysics Conference on High Energy Physics, EPS 2003, Aachen, Germany (July 17-23, 2003).

Scientific paper

10.1140/epjcd/s2003-03-1108-5

One of the most dramatic consequences of low-scale (~1 TeV) quantum gravity would be copious production of mini black holes at future accelerators and in ultra-high-energy cosmic ray interactions. Hawking radiation of these black holes is constrained mainly to our (3+1)-dimensional world and results in their rapid evaporation. We review selected topics in the mini-black-hole phenomenology, such as production rates at colliders and in cosmic rays, Hawking radiation as a sensitive probe of the dimensionality of extra space, as well as an exciting possibility of finding new physics in the decays of black holes.

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