Probing TeV gravity at neutrino telescopes
| dc.creator | Illana, J. I. | |
| dc.creator | Masip, M. | |
| dc.creator | Meloni, D. | |
| dc.date | 2006-12-22 | |
| dc.date.accessioned | 2026-07-07T07:36:47Z | |
| dc.date.available | 2026-07-07T07:36:47Z | |
| dc.description | 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. | |
| dc.description | 5 pages; to appear in the proceedings of the Workshop on Exotic Physics with Neutrino Telesocpes, Uppsala 20-22 September 2006 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0612305 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0612305 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/120550 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Probing TeV gravity at neutrino telescopes | |
| dc.type | text |