On Black Hole Detection with the OWL/Airwatch Telescope

Details On Black Hole Detection with the OWL/Airwatch Telescope On Black Hole Detection with the OWL/Airwatch Telescope

2002-04-18

arxiv.org/abs/hep-ph/0204218v2

Phys.Rev. D66 (2002) 033002

Physics

High Energy Physics

High Energy Physics - Phenomenology

8 pages, including 7 color figures, three figure captions corrected, minor changes for clarification, one reference added

Scientific paper

10.1103/PhysRevD.66.033002

In scenarios with large extra dimensions and TeV scale gravity ultrahigh energy neutrinos produce black holes in their interactions with the nucleons. We show that ICECUBE and OWL may observe large number of black hole events and provide valuable information about the fundamental Planck scale and the number of extra dimensions. OWL is especially well suited to observe black hole events produced by neutrinos from the interactions of cosmic rays with the 3 K background radiation. Depending on the parameters of the scenario of large extra dimensions and on the flux model, as many as 28 events per year are expected for a Planck scale of 3 TeV.

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