Inflating, Warming Up, and Probing the Pre-Bangian Universe
| dc.creator | Veneziano, G. | |
| dc.date | 1999-02-12 | |
| dc.date | 1999-02-17 | |
| dc.date.accessioned | 2026-07-07T04:25:58Z | |
| dc.date.available | 2026-07-07T04:25:58Z | |
| dc.description | Classical and quantum gravitational instabilities, can, respectively, inflate and warm up a primordial Universe satisfying a superstring-motivated principle of "Asymptotic Past Triviality". A physically viable big bang is thus generated without invoking either large fine-tunings or a long period of post-big bang inflation. Properties of the pre-bangian Universe can be probed through its observable relics, which include: i) a (possibly observable) stochastic gravitational-wave background; ii) a (possible) new mechanism for seeding the galactic magnetic fields; iii) a (possible) new source of large-scale structure and CMB anisotropy. | |
| dc.description | Latex file, 17 pages, 5 figures, Based on two recent talks, References updated | |
| dc.identifier | https://arxiv.org/abs/hep-th/9902097 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9902097 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/55937 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Inflating, Warming Up, and Probing the Pre-Bangian Universe | |
| dc.type | text |