Warm inflationary model in loop quantum cosmology

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

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15 pages, 1 figure, Accepted for publication in Phys. Rev. D

Scientific paper

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, $V(\phi)\propto \phi^2$, we develop a model where the
dissipation coefficient $\Gamma=\Gamma_0=$ constant. We use recent astronomical
observations for constraining the parameters appearing in our model.

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