Bouncing brane cosmologies from warped string compactifications

被引:0
|
作者
Kachru, S [1 ]
McAllister, L
机构
[1] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[2] Stanford Univ, Stanford Linear Accelerator Ctr, Stanford, CA 94305 USA
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关键词
D-branes; cosmology of theories beyond the SM;
D O I
暂无
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
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摘要
We study the cosmology induced on a brane probing a warped throat region in a Calabi-Yau compactification of type-IIB string theory. For the case of a BPS D3-brane probing the Klebanov-Strassler warped deformed conifold, the cosmology described by a suitable brane observer is a bouncing, spatially flat Friedmann-Robertson-Walker universe with time-varying Newton's constant, which passes smoothly from a contracting to an expanding phase. In the Klebanov-Tseytlin approximation to the Klebanov-Strassler solution the cosmology would end with a big crunch singularity. In this sense, the warped deformed conifold provides a string theory resolution of a spacelike singularity in the brane cosmology. The four-dimensional effective action appropriate for a brane observer is a simple scalar-tensor theory of gravity. In this description of the physics, a bounce is possible because the relevant energy-momentum tensor can classically violate the null energy condition.
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页数:18
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