Supersymmetric Candidates for Dark Matter (in German)
| dc.creator | Steffen, Frank Daniel | |
| dc.date | 2007-08-27 | |
| dc.date.accessioned | 2026-07-07T08:25:53Z | |
| dc.date.available | 2026-07-07T08:25:53Z | |
| dc.description | The identity of dark matter is one of the greatest puzzles of our Universe. Its solution may be associated with supersymmetry which is a fundamental space-time symmetry that has not been verified experimentally so far. In many supersymmetric extensions of the Standard Model of particle physics, the lightest supersymmetric particle cannot decay and is hence a promising dark matter candidate. The lightest neutralino, which appears already in the minimal supersymmetric model, can be identified as such a candidate in indirect and direct dark matter searches and at future colliders. As the superpartner of the graviton, the gravitino is another candidate for the lightest superparticle that provides a compelling explanation of dark matter. While it will neither be detected in indirect or direct searches nor be produced directly at accelerators, the analysis of late-decaying charged particles can allow for an experimental identification of the gravitino at future accelerators. In this way, the upcoming experiments at the CERN Large Hadron Collider may become a key to the understanding of our Universe. | |
| dc.description | 14 pages, 4 figures, to appear in the Jahrbuch 2007 (German only) of the Max Planck Society | |
| dc.identifier | https://arxiv.org/abs/0708.3600 | |
| dc.identifier | http://arxiv.org/abs/0708.3600 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/136766 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Experiment | |
| dc.subject | Popular Physics | |
| dc.title | Supersymmetric Candidates for Dark Matter (in German) | |
| dc.type | text |