Recent Constraints on Models of Quintessence
| dc.creator | Doran, Michael | |
| dc.date | 2003-10-15 | |
| dc.date.accessioned | 2026-07-07T02:10:26Z | |
| dc.date.available | 2026-07-07T02:10:26Z | |
| dc.description | We perform a comparison of the WMAP measurements with the predictions of quintessence cosmological models of dark energy. We consider a wide range of quintessence models, including: a constant equation-of-state; a simply-parametrized, time-evolving equation-of-state; a class of models of early quintessence; scalar fields with an inverse-power law potential. We also provide a joint fit to the CBI and ACBAR CMB data, and the type 1a supernovae. | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0310400 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0310400 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6740 | |
| dc.subject | Astrophysics | |
| dc.title | Recent Constraints on Models of Quintessence | |
| dc.type | text |