Thermal history of the string universe

Details Thermal history of the string universe Thermal history of the string universe

1992-05-27

arxiv.org/abs/hep-th/9205096v1

Phys.Rev. D46 (1992) 2366-2380

Physics

High Energy Physics

High Energy Physics - Theory

39 pages, no figures, use revtex.sty, aps.sty, aps10.sty & preprint.sty

Scientific paper

10.1103/PhysRevD.46.2366

Thermal history of the string universe based on the Brandenberger and Vafa's scenario is examined. The analysis thereby provides a theoretical foundation of the string universe scenario. Especially the picture of the initial oscillating phase is shown to be natural from the thermodynamical point of view. A new tool is employed to evaluate the multi state density of the string gas. This analysis points out that the well-known functional form of the multi state density is not applicable for the important region $T \leq T_H$, and derives a correct form of it.

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