Warm-Logamediate inflationary universe model

Abstract

Warm inflationary universe models in the context of logamediate expansion are studied. General conditions required for these models to be realizable and discussed. This study is done in the weak and strong dissipative regimes. The parameters of our models are constrained from the observational data.

16 pages, 2 figures. Accepted for publication in IJMPD. arXiv admin note: text overlap with arXiv:1108.1371

References in corpus (7)

• Warm Inflation and its Microphysical Basis
• Dynamics of Logamediate Inflation
• Cosmological perturbations in warm inflationary models with viscous pressure
• Enhanced polarization of CMB from thermal gravitational waves
• Warm inflation in the DGP brane-world model
• Warm hilltop inflation
• Kinks of open superstring field theory

Cited by in corpus (15)

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• Power spectrum for inflation models with quantum and thermal noises
• Intermediate-Generalized Chaplygin Gas inflationary universe model
• General dissipative coefficient in warm intermediate and logamediate inflation
• Supergravity Inflation with Broken Shift Symmetry and Large Tensor-to-Scalar Ratio
• Warm Inflection
• General dissipative coefficient in warm intermediate inflation in loop quantum cosmology in light of Planck and BICEP2
• Warm intermediate inflation in the Randall-Sundrum II model in the light of Planck 2015 and BICEP2 results: A general dissipative coefficient
• Reconstructing warm inflation
• Warm intermediate inflationary Universe model in the presence of a Generalized Chaplygin Gas
• Tachyon-Warm Intermediate and Logamediate Inflation in the Brane-World Model in the Light of Planck Data
• On the consistency of tachyon warm inflation with viscous pressure
• Intermediate inflation on the brane and warped DGP models
• Logamediate Inflation by Tachyon Field
• Inflationary Weak Anisotropic Model with General Dissipation Coefficient