Updated RICE Bounds on Ultrahigh Energy Neutrino fluxes and interactions

Details Updated RICE Bounds on Ultrahigh Energy Neutrino fluxes and interactions Updated RICE Bounds on Ultrahigh Energy Neutrino fluxes and interactions

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..apr.i7008h&link_type=abstract

American Physical Society, APS April Meeting, April 22-26, 2006, abstract #I7.008

Astronomy and Astrophysics

Astrophysics

Scientific paper

We explore limits on low scale gravity models set by results from the Radio Ice Cherenkov Experiment's (RICE) ongoing search for cosmic ray neutrinos in the cosmogenic, or GZK, energy range. The bound on, MD, the fundamental scale of gravity, depends upon cosmogenic flux model, black hole formation and decay treatments, inclusion of graviton mediated elastic neutrino processes, and the number of large extra dimensions, d. We find bounds in the interval 0.9 TeV < MD < 10 TeV. Values d = 5, 6 and 7, for which laboratory and astrophysical bounds on LSG models are less restrictive, lead to essentially the same limits on MD.

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