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arXiv · 1006.1299

Warm inflationary model in loop quantum cosmology

Ramon Herrera
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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, $V(ϕ)\propto ϕ^2$, we develop a model where the dissipation coefficient $Γ=Γ_0=$ constant. We use recent astronomical observations for constraining the parameters appearing in our model.

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Ramon Herrera. 2010-06-07. Warm inflationary model in loop quantum cosmology. https://doi.org/10.1103/physrevd.81.123511

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