Class of viable modified $f(R)$ gravities describing inflation and the onset of accelerated expansion
| dc.creator | Cognola, G. | |
| dc.creator | Elizalde, E. | |
| dc.creator | Nojiri, S. | |
| dc.creator | Odintsov, S. D. | |
| dc.creator | Sebastiani, L. | |
| dc.creator | Zerbini, S. | |
| dc.date | 2007-12-24 | |
| dc.date | 2008-01-30 | |
| dc.date.accessioned | 2026-07-07T11:13:55Z | |
| dc.date.available | 2026-07-07T11:13:55Z | |
| dc.description | A general approach to viable modified $f(R)$ gravity is developed in both the Jordan and the Einstein frames. A class of exponential, realistic modified gravities is introduced and investigated with care. Special focus is made on step-class models, most promising from the phenomenological viewpoint and which provide a natural way to classify all viable modified gravities. One- and two-steps models are explicitly considered, but the analysis is extensible to $N$-step models. Both inflation in the early universe and the onset of recent accelerated expansion arise in these models in a natural, unified way. Moreover, it is demonstrated that models in this category easily pass all local tests, including stability of spherical body solution, non-violation of Newton's law, and generation of a very heavy positive mass for the additional scalar degree of freedom. | |
| dc.description | 15 pages, 2 figures, version to appear in Physical Review D | |
| dc.identifier | https://arxiv.org/abs/0712.4017 | |
| dc.identifier | http://arxiv.org/abs/0712.4017 | |
| dc.identifier | Phys.Rev.D77:046009,2008 | |
| dc.identifier | doi:10.1103/PhysRevD.77.046009 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/191889 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Class of viable modified $f(R)$ gravities describing inflation and the onset of accelerated expansion | |
| dc.type | text |