The Passage of Ultrarelativistic Neutralinos through the Matter of the Moon
| dc.creator | Bornhauser, Sascha | |
| dc.date | 2008-09-29 | |
| dc.date.accessioned | 2026-07-07T12:36:16Z | |
| dc.date.available | 2026-07-07T12:36:16Z | |
| dc.description | I consider the prospect to use the outer layer of the Moon as a detector volume for ultra-high energy (UHE) neutrino fluxes and the flux of the lightest neutralino which I assume is the lightest supersymmetric particle (LSP). For this purpose, I calculate the event rates of these fluxes for top-down scenarios. I show that a suitable experiment for the detection of radio waves might be able to detect sufficient event rates after a measurement period of one year. | |
| dc.description | 3 pages, 1 figure, to appear in the proceedings of 16th International Conference on Supersymmetry and the Unification of Fundamental Interactions (SUSY08), Seoul, Korea, June 16-21 2008 | |
| dc.identifier | https://arxiv.org/abs/0809.5014 | |
| dc.identifier | http://arxiv.org/abs/0809.5014 | |
| dc.identifier | AIP Conf.Proc.1078:512-514,2009 | |
| dc.identifier | doi:10.1063/1.3052012 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/218038 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | The Passage of Ultrarelativistic Neutralinos through the Matter of the Moon | |
| dc.type | text |