Cosmological Model for the Very Early Universe in B.D. Theory
| dc.creator | Berman, Marcelo Samuel | |
| dc.date | 2006-05-17 | |
| dc.date.accessioned | 2026-07-07T07:09:44Z | |
| dc.date.available | 2026-07-07T07:09:44Z | |
| dc.description | Following a paper by Berman and Marinho Jr (2001), where it was established an equation of state (p=-(1/3)rho), for the very early Universe, under which, Einstein's equations with lambda=0, render a scale-factor proportional to the time coordinate, and under which, Berman(2006, 2006a) showed that in the non-null lambda case, the Universe entered automatically into an exponential inflationary phase, we now study the corresponding effect in Brans-Dicke Cosmology. We find that the resulting models are similar to those in General Relativity Cosmology. | |
| dc.description | 5 pages including front page. To be submitted to Astrophysics and Space Science | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0605092 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0605092 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/111185 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Cosmological Model for the Very Early Universe in B.D. Theory | |
| dc.type | text |