Temperature in warm inflation in non-minimal kinetic coupling model

Warm inflation in the non-minimal derivative coupling model with a general dissipative coefficient is considered. We investigate the conditions for the existence of the slow roll approximation and study cosmological perturbations. The spectral index and the power spectrum are calculated and the temp...

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Bibliographic Details
Published in:The European physical journal. C, Particles and fields Particles and fields, 2015-10, Vol.75 (10), p.1-9, Article 513
Main Authors: Sadjadi, H. Mohseni, Goodarzi, Parviz
Format: Article
Language:English
Subjects:
Analysis
Approximation
Astronomy
Astrophysics and Cosmology
Coupling
Derivatives
Elementary Particles
Hadrons
Heavy Ions
Inflation
Inflation (Finance)
Mathematical analysis
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Perturbation methods
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article - Theoretical Physics
Rolls
Spectra
String Theory
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Summary:Warm inflation in the non-minimal derivative coupling model with a general dissipative coefficient is considered. We investigate the conditions for the existence of the slow roll approximation and study cosmological perturbations. The spectral index and the power spectrum are calculated and the temperature of the universe at the end of the slow roll warm inflation is obtained.
ISSN:1434-6044
1434-6052
DOI:10.1140/epjc/s10052-015-3745-6