Abstract
We present a detailed study of a recently proposed model for primordial inflation based on an N=1 locally supersymmetric potential. For a large class of parameters with which all cosmological constraints are satisfied, the temperature corrections can be neglected during the inflation period. At higher temperatures, the minimum is not at the origin, but very close to it.
Original language | English (US) |
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Pages (from-to) | 53-58 |
Number of pages | 6 |
Journal | Physics Letters B |
Volume | 131 |
Issue number | 1-3 |
DOIs | |
State | Published - Nov 10 1983 |