Inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills-$F(R)$ gravity and non-minimal vector-$F(R)$ gravity
| dc.creator | Bamba, Kazuharu | |
| dc.creator | Nojiri, Shin'ichi | |
| dc.creator | Odintsov, Sergei D. | |
| dc.date | 2008-03-24 | |
| dc.date | 2008-06-05 | |
| dc.date.accessioned | 2026-07-07T11:49:18Z | |
| dc.date.available | 2026-07-07T11:49:18Z | |
| dc.description | We study inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills (YM) theory, in which the YM field couples to a function of the scalar curvature. It is shown that power-law inflation can be realized due to the non-minimal YM field-gravitational coupling which maybe caused by quantum corrections. Moreover, it is demonstrated that both inflation and the late-time accelerated expansion of the universe can be realized in a modified YM-$F(R)$ gravity which is consistent with solar system tests. Furthermore, it is shown that this result can be realized also in a non-minimal vector-$F(R)$ gravity. In addition, we consider the duality of the non-minimal electromagnetic theory and that of the non-minimal YM theory, and also discuss the cosmological reconstruction of the YM theory. | |
| dc.description | 21 pages, no figure, shortened version, accepted in PRD, misprints corrected | |
| dc.identifier | https://arxiv.org/abs/0803.3384 | |
| dc.identifier | http://arxiv.org/abs/0803.3384 | |
| dc.identifier | Phys.Rev.D77:123532,2008 | |
| dc.identifier | doi:10.1103/PhysRevD.77.123532 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/203188 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills-$F(R)$ gravity and non-minimal vector-$F(R)$ gravity | |
| dc.type | text |