New Solutions of the Inflationary Flow Equations
| dc.creator | Spalinski, Michal | |
| dc.date | 2007-06-18 | |
| dc.date | 2007-06-27 | |
| dc.date.accessioned | 2026-07-07T11:16:56Z | |
| dc.date.available | 2026-07-07T11:16:56Z | |
| dc.description | The inflationary flow equations are a frequently used method of surveying the space of inflationary models. In these applications the infinite hierarchy of differential equations is truncated in a way which has been shown to be equivalent to restricting the set of models considered to those characterized by polynomial inflaton potentials. This paper explores a different method of solving the flow equations, which does not truncate the hierarchy and in consequence covers a much wider class of models while retaining the practical usability of the standard approach. | |
| dc.description | References added, and a couple of comments | |
| dc.identifier | https://arxiv.org/abs/0706.2503 | |
| dc.identifier | http://arxiv.org/abs/0706.2503 | |
| dc.identifier | JCAP0708:016,2007 | |
| dc.identifier | doi:10.1088/1475-7516/2007/08/016 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/192844 | |
| dc.subject | Astrophysics | |
| dc.title | New Solutions of the Inflationary Flow Equations | |
| dc.type | text |