arXiv · gr-qc/0005072
Primordial fluctuations of the metric in the warm inflation scenario
Abstract
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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Mauricio Bellini. 2000-05-16. Primordial fluctuations of the metric in the warm inflation scenario. https://arxiv.org/abs/gr-qc/0005072
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