Gauge Couplings at High Temperature and the Relic Gravitino Abundance
| dc.creator | Buchmüller, W. | |
| dc.creator | Hamaguchi, K. | |
| dc.creator | Ratz, M. | |
| dc.date | 2003-07-14 | |
| dc.date | 2003-09-04 | |
| dc.date.accessioned | 2026-07-07T11:31:26Z | |
| dc.date.available | 2026-07-07T11:31:26Z | |
| dc.description | In higher-dimensional supersymmetric theories gauge couplings of the effective four-dimensional theory are determined by expectation values of scalar fields. We find that at temperatures above a critical temperature $T_*$, which depends on the supersymmetry breaking mass scales, gauge couplings decrease like $T^{-\a}$, $\a > 1$. This has important cosmological consequences. In particular it leads to a relic gravitino density which becomes independent of the reheating temperature for $T_R > T_*$. For small gravitino masses, $m_{3/2} \ll m_{\gl}$, the mass density of stable gravitinos is essentially determined by the gluino mass. The observed value of cold dark matter, $Ø_{\rm CDM}h^2 \sim 0.1$, is obtained for gluino masses $m_{\gl} = {\cal O}(1 {\rm TeV})$. | |
| dc.description | 11 pages, 2 figures, comment on supersymmetry breaking mechanisms and two references added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0307181 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0307181 | |
| dc.identifier | Phys.Lett.B574:156-161,2003 | |
| dc.identifier | doi:10.1016/j.physletb.2003.09.017 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197269 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Gauge Couplings at High Temperature and the Relic Gravitino Abundance | |
| dc.type | text |