Warm inflationary model in loop quantum cosmology

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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
Issue number12
StatePublished - 2010


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