DILATON-DRIVEN INFLATION IN STRING COSMOLOGY
| dc.creator | Brustein, Ram | |
| dc.date | 1995-06-07 | |
| dc.date.accessioned | 2026-07-07T04:21:14Z | |
| dc.date.available | 2026-07-07T04:21:14Z | |
| dc.description | I present an outline for cosmological evolution in the framework of string theory with emphasis on a phase of dilaton-driven kinetic inflation. It is shown that a typical background of stochastic gravitational radiation is generated, with strength that may allow its detection in future gravity wave experiments. | |
| dc.description | 11 pages, latex, 1 figure icluded as an epsf file | |
| dc.identifier | https://arxiv.org/abs/hep-th/9506045 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9506045 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/54236 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | DILATON-DRIVEN INFLATION IN STRING COSMOLOGY | |
| dc.type | text |