Gravitino and Axino SuperWIMPs
| dc.creator | Cembranos, J. A. R. | |
| dc.creator | Feng, Jonathan L. | |
| dc.creator | Rajaraman, A. | |
| dc.creator | Takayama, F. | |
| dc.date | 2007-01-01 | |
| dc.date.accessioned | 2026-07-07T10:22:15Z | |
| dc.date.available | 2026-07-07T10:22:15Z | |
| dc.description | Gravitinos and axinos produced in the late decays of other supersymmetric particles are well-motivated dark matter (DM) candidates, whose experimental evidences are very distinctive and different from other standard candidates, as thermal produced neutralinos in similar supersymmetric models. In particular, charged sleptons could appear stable because of the length of its lifetime. The direct production of such particles at both the Large Hadron Collider (LHC) and a future International Linear Collider (ILC) can give not only a clear signature of supersymmetry but also the first non-gravitational evidence of dark matter. | |
| dc.description | 4 pages, LaTeX, 1 figure, Updated references. To appear in Proceedings of SUSY06, the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0701011 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0701011 | |
| dc.identifier | AIPConf.Proc.903:591-594,2007 | |
| dc.identifier | doi:10.1063/1.2735254 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/175455 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Gravitino and Axino SuperWIMPs | |
| dc.type | text |