Reheat temperature in supersymmetric hybrid inflation models
| dc.creator | Senoguz, V. N. | |
| dc.creator | Shafi, Q. | |
| dc.date | 2004-12-07 | |
| dc.date | 2005-02-25 | |
| dc.date.accessioned | 2026-07-07T10:29:21Z | |
| dc.date.available | 2026-07-07T10:29:21Z | |
| dc.description | The allowed range of parameters for supersymmetric hybrid inflation and its extensions are investigated. The lower bound on the reheat temperature T_r in these models with hierarchical right handed neutrinos is found to be 3*10^7 GeV. (T_r as low as 100 GeV is possible for quasi degenerate right handed neutrinos.) We also present revised estimates for the scalar spectral index and the symmetry breaking scale associated with inflation. | |
| dc.description | 15 pages, 8 figures, revtex4. v2: minor changes, matches published version | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0412102 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0412102 | |
| dc.identifier | Phys.Rev.D71:043514,2005 | |
| dc.identifier | doi:10.1103/PhysRevD.71.043514 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177768 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Reheat temperature in supersymmetric hybrid inflation models | |
| dc.type | text |