Modified non-local-F(R) gravity as the key for the inflation and dark energy
| dc.creator | Nojiri, Shin'ichi | |
| dc.creator | Odintsov, Sergei D. | |
| dc.date | 2007-08-07 | |
| dc.date | 2007-12-03 | |
| dc.date.accessioned | 2026-07-07T11:18:29Z | |
| dc.date.available | 2026-07-07T11:18:29Z | |
| dc.description | We consider FRW cosmology in non-local modified gravity. Its local scalar-tensor formulation is developed. It is explicitly demonstrated that such theory may lead to the unification of early-time inflation with late-time cosmic acceleration. The quintessence or phantom era may emerge for specific form of the action. The coupled non-local-F(R) gravity is also investigated. It is shown that such theory being consistent with Solar System tests may lead to the known universe history sequence: inflation, radiation/matter dominance and dark epoch. | |
| dc.description | LaTeX file, 9 pages, version to appear in PLB | |
| dc.identifier | https://arxiv.org/abs/0708.0924 | |
| dc.identifier | http://arxiv.org/abs/0708.0924 | |
| dc.identifier | Phys.Lett.B659:821-826,2008 | |
| dc.identifier | doi:10.1016/j.physletb.2007.12.001 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/193362 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Modified non-local-F(R) gravity as the key for the inflation and dark energy | |
| dc.type | text |