Warm intermediate inflation in the Randall–Sundrum II model in the light of Planck 2015 and BICEP2 results: a general dissipative coefficient

A warm inflationary Universe in the Randall–Sundrum II model during intermediate inflation is studied. For this purpose, we consider the general form for the dissipative coefficient Γ ( T , ϕ ) = C ϕ T m ϕ m - 1 , and also we analyze this inflationary model in the weak and strong dissipative regimes...

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Bibliographic Details
Published in:The European physical journal. C, Particles and fields Particles and fields, 2015-05, Vol.75 (5), p.1, Article 205
Main Authors: Herrera, Ramón, Videla, Nelson, Olivares, Marco
Format: Article
Language:English
Subjects:
Analysis
Astronomy
Astrophysics and Cosmology
Elementary Particles
Hadrons
Heavy Ions
Inflation (Finance)
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Regular Article - Theoretical Physics
String Theory
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Summary:A warm inflationary Universe in the Randall–Sundrum II model during intermediate inflation is studied. For this purpose, we consider the general form for the dissipative coefficient Γ ( T , ϕ ) = C ϕ T m ϕ m - 1 , and also we analyze this inflationary model in the weak and strong dissipative regimes. We study the evolution of the Universe under the slow-roll approximation and find solutions to the full effective Friedmann equation in the brane-world framework. In order to constrain the parameters in our model, we consider the recent data from the BICEP2 to Planck 2015 data together with the necessary condition for warm inflation T > H , and also the condition from the weak (or strong) dissipative regime.
ISSN:1434-6044
1434-6052
DOI:10.1140/epjc/s10052-015-3433-6