The dynamics of scalar fields in the inflationary universe

Details The dynamics of scalar fields in the inflationary universe The dynamics of scalar fields in the inflationary universe

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phya..158..343b&link_type=abstract

Physica A, Volume 158, Issue 1, p. 343-358.

Physics

3

Scientific paper

The evolution of weakly coupled scalar fields in the early universe is discussed. Such fields will be out of thermal equilibrium, and their initial distribution will be inhomogeneous. We study the classical evolution in a pre-inflationary radiation dominated universe and discuss under which conditions the fields dynamically relax to configurations which gave inflation.

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