"Soft bang" instead of "big bang": model of an inflationary universe without singularities and with eternal physical past time
| dc.creator | Rebhan, E. | |
| dc.date | 2006-02-23 | |
| dc.date.accessioned | 2026-07-07T07:00:51Z | |
| dc.date.available | 2026-07-07T07:00:51Z | |
| dc.description | The solution for an inflationary universe without singularities is derived from the Einstein-Lemaitre equations. The present state of the universe evolved from a steady state solution for a tiny, but classical micro-universe with large cosmological constant or large equivalent vacuum energy density and with an equal energy density of radiation and/or some kind of relativistic primordial matter in the infinite past. An instability of this state outside the quantum regime caused a "soft bang" by triggering an expansion that smoothly started with zero expansion rate, continuously increased, culminated in an exponentially inflating phase and ended through a phase transition, the further evolution being a Friedmann-Lemaitre evolution as in big bang models. As a necessary implication of the model the universe must be closed. All other parameters of the model are very similar to those of big bang models and comply with observational constraints. | |
| dc.description | 21 pages, 5 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0602515 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0602515 | |
| dc.identifier | Astron.Astrophys. 353 (2000) 1-9 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/108102 | |
| dc.subject | Astrophysics | |
| dc.title | "Soft bang" instead of "big bang": model of an inflationary universe without singularities and with eternal physical past time | |
| dc.type | text |