Abstract

There has recently been considerable interest in inflationary scenarious for the very early universe. 0.2) In this respect the de Sitter solution plays a crucial role as a cosmological model with a positive cosmological constant A.3) However, to overcome some fundamental difficulties with these concepts some super­ symmetric inflationary models or super­ cosmologies have been proposed.')-'B) It seems now probable that the new scenario of an inflating or chaotic universe can be completely realized within the framework of N = 1 supergravity. The state of the art has been recently reviewed by Linde. '9) Furthermore, exact supergravity cosmological solutions have been recently constructed by Freund/O) Gleiser et al.,20,22) Chapline and Gibbons,23) Myung and Kim/

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