Warm-Intermediate inflationary universe model in braneworld cosmologies
General Relativity and Quantum Cosmology
2011-12-25 v1 Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
Abstract
Warm-intermediate inflationary universe models in the context of braneworld cosmologies, are studied. This study is done in the weak and strong dissipative regimes. We find that, the scalar potentials and dissipation coefficients in terms of the scalar field, evolves as type-power-law and powers of logarithms, respectively. General conditions required for these models to be realizable are derived and discussed. We also study the scalar and tensor perturbations for each regime. We use recent astronomical observations to constraint the parameters appearing in the braneworld models.
Cite
@article{arxiv.1108.1371,
title = {Warm-Intermediate inflationary universe model in braneworld cosmologies},
author = {Ramon Herrera and Eugenio San Martin},
journal= {arXiv preprint arXiv:1108.1371},
year = {2011}
}
Comments
19 pages, 2 figures. Published in Eur. Phys. J. C. arXiv admin note: substantial overlap with arXiv:0903.4214 and arXiv:1003.5645