Constraints on Supergravity Chaotic Inflationary Models
arXiv:gr-qc/9507045 · doi:10.1016/0370-2693(95)01169-2
Abstract
We discuss, in the context of hidden sector non-minimal supergravity chaotic inflationary models, constraints on the parameters of a polynomial superpotential resulting from existing bounds on the reheating temperature and on the amplitude of the primordial energy density fluctuations as inferred from COBE. We present a specific two-parameter chaotic inflationary model which satisfies these constraints and discuss a possible scenario for adequate baryon asymmetry generation.
Latex file, 10 pages; important changes and references added
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