Authors: Suayyip Salim Ozkurt
The inflationary phase of the evolution of the ten dimensional universe is considered. The form of the stress-energy tensor of the matter in the very early universe is determined by making use of some thermodynamical arguments. In this way, the Einstein field equations are written and some inflationary cosmological solution is found to these equations in which, while the actual dimensions are exponentially expanding, the others are contracting.
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[v1] 28 Dec 2007
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