| Full text | |
| Author(s): |
Total Authors: 2
|
| Affiliation: | [1] Inst Tecnol Aeronaut, Dept Fis, BR-12228900 Sao Jose Dos Campos, SP - Brazil
[2] Univ Fed Campina Grande, Dept Fis, BR-58109970 Campina Grande, Paraiba - Brazil
Total Affiliations: 2
|
| Document type: | Journal article |
| Source: | EUROPEAN PHYSICAL JOURNAL C; v. 76, n. 2 FEB 4 2016. |
| Web of Science Citations: | 23 |
| Abstract | |
Recent elaborated by Harko et al., the f(R, T) theories of gravity allow one to contemplate an optimistic alternative to dark energy, for which R and T stand for the Ricci scalar and the trace of the energy-momentum tensor, respectively. Although the literature has shown that the T dependence on the gravitational part of the action - which is due to the consideration of quantum effects - may induce some novel features in the scope of late-time cosmological dynamics, in the radiation-dominated universe, when T = 0, no contributions seem to arise from such theories. Apparently, f(R, T) contributions to a radiation-dominated universe may arise only from the f(R, T-phi) approach, which is nothing but the f(R, T) gravity in the case of a self-interacting scalar field whose trace of the energy-momentum tensor is T-phi. We intend, in this article, to show how f(R, T-phi) theories of gravity can contribute to the study of the primordial stages of the universe. Our results predict a graceful exit from an inflationary stage to a radiation-dominated era. They also predict a late-time cosmic acceleration after a matter-dominated phase, enabling the f(R, T-phi) theories to describe, in a self-consistent way, all the different stages of the dynamics of the universe. (AU) | |
| FAPESP's process: | 15/08476-0 - Gravitational waves in f(R,T) theories: polarization states and astrophysical sources |
| Grantee: | Pedro Henrique Ribeiro da Silva Moraes |
| Support type: | Scholarships in Brazil - Post-Doctorate |