Dark energy in modified Gauss-Bonnet gravity: late-time acceleration and the hierarchy problem
| dc.creator | Cognola, Guido | |
| dc.creator | Elizalde, Emilio | |
| dc.creator | Nojiri, Shin'ichi | |
| dc.creator | Odintsov, Sergei D. | |
| dc.creator | Zerbini, Sergio | |
| dc.date | 2005-12-31 | |
| dc.date | 2006-03-01 | |
| dc.date.accessioned | 2026-07-07T11:06:25Z | |
| dc.date.available | 2026-07-07T11:06:25Z | |
| dc.description | Dark energy cosmology is considered in a modified Gauss-Bonnet (GB) model of gravity where an arbitrary function of the GB invariant, $f(G)$, is added to the General Relativity action. We show that such theory is endowed with a quite rich cosmological structure: it may naturally lead to an effective cosmological constant, quintessence or phantom cosmic acceleration, with a possible transition from deceleration to acceleration. It is demonstrated in the paper that this theory is perfectly viable, since it is compliant with Solar System constraints. Specific properties of $f(G)$ gravity in a de Sitter universe, such as dS and SdS solutions, their entropy and its explicit one-loop quantization are studied. The issue of a possible solution of the hierarchy problem in modified gravities is addressed too. | |
| dc.description | LaTeX file 20 pages, new subsections are added | |
| dc.identifier | https://arxiv.org/abs/hep-th/0601008 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0601008 | |
| dc.identifier | Phys.Rev.D73:084007,2006 | |
| dc.identifier | doi:10.1103/PhysRevD.73.084007 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/189514 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Dark energy in modified Gauss-Bonnet gravity: late-time acceleration and the hierarchy problem | |
| dc.type | text |