中文

de Sitter Vacua in String Theory

高能物理 - 理论 2008-11-26 v2 天体物理学 广义相对论与量子宇宙学 高能物理 - 唯象学

摘要

We outline the construction of metastable de Sitter vacua of type IIB string theory. Our starting point is highly warped IIB compactifications with nontrivial NS and RR three-form fluxes. By incorporating known corrections to the superpotential from Euclidean D-brane instantons or gaugino condensation, one can make models with all moduli fixed, yielding a supersymmetric AdS vacuum. Inclusion of a small number of anti-D3 branes in the resulting warped geometry allows one to uplift the AdS minimum and make it a metastable de Sitter ground state. The lifetime of our metastable de Sitter vacua is much greater than the cosmological timescale of 10^10 years. We also prove, under certain conditions, that the lifetime of dS space in string theory will always be shorter than the recurrence time.

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引用

@article{arxiv.hep-th/0301240,
  title  = {de Sitter Vacua in String Theory},
  author = {Shamit Kachru and Renata Kallosh and Andrei Linde and Sandip P. Trivedi},
  journal= {arXiv preprint arXiv:hep-th/0301240},
  year   = {2008}
}

备注

12 pages, 2 figs, added comments on the thin wall approximation to tunneling