Hagedorn inflation of D-branes

Details Hagedorn inflation of D-branes Hagedorn inflation of D-branes

2000-05-03

arxiv.org/abs/hep-th/0005028v1

JHEP 0101:039,2001

Physics

High Energy Physics

High Energy Physics - Theory

44 Pages; JHEP latex; includes 1 postscript figure

Scientific paper

10.1088/1126-6708/2001/01/039

We examine the cosmological effects of the Hagedorn phase in models where the observable universe is pictured as a D-brane. It is shown that, even in the absence of a cosmological constant, winding modes cause a negative `pressure' that can drive brane inflation of various types including both power law and exponential. We also find regimes in which the cosmology is stable but oscillating (a bouncing universe) with the Hagedorn phase softening the singular behavior associated with the collapse.

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