Detecting TeV Black Holes from Extensive Air Showers

Details Detecting TeV Black Holes from Extensive Air Showers Detecting TeV Black Holes from Extensive Air Showers

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1515a&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

In models with large extra dimensions particle collisions with centre-of-mass energy larger than the fundamental gravitational scale can generate non-perturbative gravitational objects such as black holes and branes. They might be created in the next generation particle colliders or by neutrino induced air showers in the Earth's atmosphere. The decay of these non-perturbative gravitational objects is significantly different from other standard model processes. We present a comprehensive study of how to differentiate extensive air showers generated by TeV gravity effects from those generated by standard model interactions.

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