Curvaton reheating and intermediate inflation in brane cosmology
arXiv:1111.1304 · doi:10.1139/p11-087
Abstract
In this paper, we study the curvaton reheating mechanism for an intermediate inflationary universe in brane world cosmology. In contrast to our previous work, we assume that when the universe enters the kination era, it is still in the high-energy regime. We then discuss, in detail, the new cosmological constraints on both the model parameters and the physical quantities.
15 pages, 4 figures. With some modifications to the text the version published on Can. J. Phys. arXiv admin note: significant text overlap with arXiv:1011.0801
References in corpus (10)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Curvaton reheating allows TeV Hubble scale in NO inflation
- Intermediate inflation on the brane
- Curvaton reheating in logamediate inflationary model
- Non-canonical generalizations of slow-roll inflation models
- Curvaton field and intermediate inflationary universe model
- Curvaton Dynamics in Brane-worlds
- The curvaton scenario in Brane cosmology: model parameters and their constraints