MSSM: source for generating perturbations
| dc.creator | Mazumdar, A. | |
| dc.date | 2004-02-01 | |
| dc.date.accessioned | 2026-07-07T03:51:55Z | |
| dc.date.available | 2026-07-07T03:51:55Z | |
| dc.description | In this talk I describe how MSSM flat directions act as a source for generating all matter and scale invariant adiabatic density perturbations with a spectral index slightly depending upon the choice of a particular flat direction. | |
| dc.description | 4 pages, To appear in the Proceedings of SUSY 2003, held at the University of Arizona, Tucson, AZ, 5-10 June 2003 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0402013 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0402013 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/43280 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | MSSM: source for generating perturbations | |
| dc.type | text |