A Model for the Big Bounce

Details A Model for the Big Bounce A Model for the Big Bounce

2003-12-16

arxiv.org/abs/hep-th/0312182v1

JCAP 0403 (2004) 004

Physics

High Energy Physics

High Energy Physics - Theory

10 pages, 2 figures

Scientific paper

10.1088/1475-7516/2004/03/004

I motivate a proposal for modeling, 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.

Affiliated with

Also associated with

No associations

Rating

A Model for the Big Bounce does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A Model for the Big Bounce, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Model for the Big Bounce will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-511402