Black Holes and Quasistable Remnants at the Lhc

Details Black Holes and Quasistable Remnants at the Lhc Black Holes and Quasistable Remnants at the Lhc

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006fuin.conf..235k&link_type=abstract

FUNDAMENTAL INTERACTIONS. Proceedings of the 21st Lake Louise Winter Institute. Held 17-23 February 2006 in Lake Louise, Alberta

Physics

Scientific paper

In models with large extra dimensions (LXDs) the Planck scale can be lowered to values that are within the reach of the next generation of particle colliders. Those models predict the production of TeV mass black holes and therefore a new era in short distance physics. However, the details of the black hole evaporation process especially in the final phase are unknown. We study the implications of the assumption that a quasi stable remnant is formed. Therefore the black hole particle spectrum and direct detection are taken into account.

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