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.
|Journal||Physical Review D - Particles, Fields, Gravitation and Cosmology|
|State||Published - 2010|