Stationary Universe Model : Inputs and Outputs 1
نویسنده
چکیده
In our opinion, the simplest and, simultaneously, the most general version of inflationary cosmology is the chaotic inflation scenario. It can be realized in all models were the other versions of inflationary theory can be realized (see [4] for detailed account). Several years ago it was realized that inflation in these theories has a very interesting property which will be discussed in this talk. If the universe contains at least one inflationary domain of a size of horizon (h-region) with a sufficiently large and homogeneous scalar field φ, then this domain will permanently produce new h-regions of a similar type. During this process the total physical volume of the inflationary universe (which is proportional to the total number of h-regions) will grow indefinitely.
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