Non-Minimal Inflation after WMAP3
| dc.creator | Nozari, Kourosh | |
| dc.creator | Sadatian, S. Davood | |
| dc.date | 2007-09-29 | |
| dc.date | 2007-10-16 | |
| dc.date.accessioned | 2026-07-07T12:21:41Z | |
| dc.date.available | 2026-07-07T12:21:41Z | |
| dc.description | The Wilkinson Microwave Anisotropy Probe (WMAP) three year results are used to constraint non-minimal inflation models. Two different non-minimally coupled scalar field potentials are considered to calculate corresponding slow-roll parameters of non-minimal inflation. The results of numerical analysis of parameter space are compared with WMAP3 data to find appropriate new constraints on the values of the non-minimal coupling. A detailed comparison of our results with previous studies reveals the present status of the non-minimal inflation model after WMAP3. | |
| dc.description | 16 pages, 11 figures, 2 tables, Revised Version | |
| dc.identifier | https://arxiv.org/abs/0710.0058 | |
| dc.identifier | http://arxiv.org/abs/0710.0058 | |
| dc.identifier | Mod.Phys.Lett.A23:2933-2945,2008 | |
| dc.identifier | doi:10.1142/S0217732308026698 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/213416 | |
| dc.subject | Astrophysics | |
| dc.title | Non-Minimal Inflation after WMAP3 | |
| dc.type | text |