The reviewed record of science sign in
Pith

arxiv: hep-ph/0612305 · v1 · pith:JOA2P4IO · submitted 2006-12-22 · hep-ph

Probing TeV gravity at neutrino telescopes

Reviewed by Pith T0 review T1 audit T2 compute T3 formal T4 kernel pith:JOA2P4IOrecord.jsonopen to challenge →

classification hep-ph
keywords neutrinoblackeventstelescopesapartapproximationcalculatedcharged
0
0 comments X
read the original abstract

Models with extra dimensions and the fundamental scale at the TeV could imply sign als in large neutrino telescopes due to gravitational scattering of cosmogenic neu trinos in the detection volume. Apart from the production of microscopic black hol es, extensively studied in the literature, we present gravity-mediated interactions at larger distances, that can be calculated in the e ikonal approximation. In these elastic processes the neutrino loses a small fracti on of energy to a hadronic shower and keeps going. The event rate of these events is higher than that of black hole formation and the signal is distinct: no charged leptons and possibly multiple-bang events.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.