A new bound on supersymmetric Q-balls
| dc.creator | Schissel, Jason | |
| dc.date | 2006-08-01 | |
| dc.date.accessioned | 2026-07-07T07:20:17Z | |
| dc.date.available | 2026-07-07T07:20:17Z | |
| dc.description | Stable baryonic Q-balls, which appear in supersymmetric extensions of the Standard Model, could form at the end of cosmological inflation from fragmentation of the Affleck-Dine condensate. They can be dark matter. The existing bounds rely on the ability of Super-Kamiokande detector to trigger on a slowly moving bright source, which may be difficult for techinical reasons. We present a weaker but more robust bound based on the flux of neutrinos produced by relic Q-balls interacting in Earth. | |
| dc.description | 7 pages | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0608014 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0608014 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/114909 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | A new bound on supersymmetric Q-balls | |
| dc.type | text |