Initial Conditions for Supersymmetric Inflation
arXiv:hep-ph/9707296 · doi:10.1103/PhysRevD.56.4562
Abstract
We perform a numerical investigation of the fields evolution in the supersymmetric inflationary model based on radiative corrections. Supergravity corrections are also included. We find that, out of all the examined initial data, only about 10% give an adequate amount of inflation and can be considered as ''natural''. Moreover, these successful initial conditions appear scattered and more or less isolated.
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