Warm inflationary model in loop quantum cosmology

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Abstract

A warm inflationary universe model in loop quantum cosmology is studied. In general we discuss the condition of inflation in this framework. By using a chaotic potential, V(φ) φ 2, we develop a model where the dissipation coefficient Γ=Γ0=constant. We use recent astronomical observations for constraining the parameters appearing in our model.

Original languageEnglish
Article number123511
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume81
Issue number12
DOIs
StatePublished - 21 Jul 2010

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