Initial Conditions in Pre-Big Bang
| dc.creator | Kaloper, Nemanja | |
| dc.date | 1998-08-12 | |
| dc.date.accessioned | 2026-07-07T04:24:56Z | |
| dc.date.available | 2026-07-07T04:24:56Z | |
| dc.description | This note is a summary of the work reported in hep-th/9801073. We give a brief discussion of the fine tuning problem in pre-big bang cosmology. We use the flatness problem as our test case, and in addition to the exact numerical limits on initial conditions, we highlight the differences between pre-big bang and standard inflation. The main difference is that in pre-big bang the universe must be smooth and flat in an exponentially large domain already at the beginning of the dilaton-driven inflation. | |
| dc.description | 5 pages, Latex with sprocl.sty, based on talks given at PASCOS-98 and CAPP-98 | |
| dc.identifier | https://arxiv.org/abs/hep-th/9808063 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9808063 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/55601 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Initial Conditions in Pre-Big Bang | |
| dc.type | text |