Intermediate inflation on the brane and warped DGP models
arXiv:1309.7954 · doi:10.1140/epjc/s10052-013-2475-x
Abstract
Brane and warped Dvali-Gabadadze-Porrati inflationary universe models in the context of intermediate inflation are studied. In both models we consider that the energy density is a standard scalar field and we discuss the evolution of the universe during the slow-roll inflation. Also, we describe the conditions for these models. The corresponding Wilkinson Microwave Anisotropy Probe seven year data are utilized to fix some parameters in our models. Our results are compared to those found in General Relativity.
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- Inflationary cosmology with Chaplygin gas in Palatini formalism
- Intermediate accelerated solutions as generic late-time attractors in a modified Jordan-Brans-Dicke theory
- Do sewn singularities falsify the Palatini cosmology?
- Warped DGP model in warm intermediate inflation with a general dissipative coefficient in light of BICEP2 and Planck results
- Dynamics of Warm Chaplygin Gas Inflationary Models With Quartic Potential
- Scalar warm inflation in holographic cosmology
- Constant-roll Inflation in Brane Induced Gravity Cosmology
- Logamediate inflation in DGP cosmology driven by a non-canonical scalar field