Warm inflation and classicality conditions

Details Warm inflation and classicality conditions Warm inflation and classicality conditions

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phlb..428...31b&link_type=abstract

Physics Letters B, Volume 428, Issue 1-2, p. 31-36.

Physics

30

Scientific paper

In this work we analize the classicality conditions that must be satisfied to have an effective stochastic approach, in the framework of warm inflation scenarios. The radiation temperature at the end of inflation is of the order of 1014 GeV, for an scalar field with mass m~(10-4-10-5) Mp, and the energy fluctuations decreases with the time. © 1998

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