Constraints on brane inflation from WMAP3
| dc.creator | Lorenz, Larissa | |
| dc.date | 2008-01-31 | |
| dc.date.accessioned | 2026-07-07T08:57:31Z | |
| dc.date.available | 2026-07-07T08:57:31Z | |
| dc.description | Considerable and ongoing effort is made to identify promising scalar field candidates in string theory to drive a cosmological period of inflation. At stake is the possibility that fundamental string parameters could be encoded in observables such as the CMB perturbation spectrum. In this contribution, we hold a concrete model of string inflation (KKLMMT) up against WMAP3 and discuss the constraints obtained. | |
| dc.description | 4 pages, 2 figures, proceedings of the workshop JGRG 17 (Nagoya, Japan, December 2007) | |
| dc.identifier | https://arxiv.org/abs/0801.4891 | |
| dc.identifier | http://arxiv.org/abs/0801.4891 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/146997 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Constraints on brane inflation from WMAP3 | |
| dc.type | text |