A Different Approach to $f(R)$-Cosmology
| dc.creator | Srivastava, S. K. | |
| dc.date | 2008-09-19 | |
| dc.date | 2008-10-09 | |
| dc.date.accessioned | 2026-07-07T10:08:24Z | |
| dc.date.available | 2026-07-07T10:08:24Z | |
| dc.description | Here $f(R)$-cosmology is discussed using a different approach. This model explains early-inflation, emergence of cosmic background radiation at the exit from inflation, cosmic deceleration during radiation-dominance followed by deceleration due to curvature-induced matter and acceleration in the very late universe due to curvature-induced phantom dark energy. This model predicts collapse in the future universe. Further, a possible avoidence of collapse as well as revival of very early universe is suggested. | |
| dc.description | This is an invited article for the anniversary volume on the occasion of 50th birthday of Prof. Sergie D. Odintsov being published by Tomsk State Pedagogical University | |
| dc.identifier | https://arxiv.org/abs/0809.3284 | |
| dc.identifier | http://arxiv.org/abs/0809.3284 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/170979 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | A Different Approach to $f(R)$-Cosmology | |
| dc.type | text |