Primordial fluctuations of the metric in the warm inflation scenario

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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Accepted for publication in Il Nuovo Cimento B, 5 pages, no figures

Scientific paper

I consider a semiclassical expansion of the scalar field in the warm
inflation scenario. I study the evolution for the fluctuations of the metric
around the Friedmann-Robertson-Walker one. The formalism predicts that, in the
power-law expansion universe, the fluctuations of the metric decreases with
time.

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