A model for the big bounce

被引：27

作者：

Veneziano, G ^{[1
]}

机构：

[1] CERN, Div Theoret Phys, CH-1211 Geneva 23, Switzerland

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2004年 / 03期

关键词：

physics of the early universe; string theory and cosmology; cosmology with extra dimensions;

D O I：

10.1088/1475-7516/2004/03/004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

I suggest a proposal for modelling, at weak string coupling, the 'Big Bounce' transition from a growing-curvature phase to standard (FRW) cosmology in terms of a pressure-less dense gas of 'string holes' (SH): string states lying on the correspondence curve between strings and black holes. During this phase SH evolve in such a way that temperature and (string-frame) curvature remain O(M-s) and (a cosmological version of) the holographic entropy bound remains saturated. This reasoning also appears to imply a new interpretation of the Hagedorn phase transition in string theory.

引用

页码：51 / 57

页数：7

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