中文

Supergravity, M theory and Cosmology

高能物理 - 理论 2007-05-23 v1 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 discuss some recent attempts to reconcile cosmology with supergravity and M/string theory. First of all, we point out that in extended supergravities the scalar masses are quantized in terms of the cosmological constant in de Sitter vacua: the eigenvalues of the Casimir operator 3 m^2/\Lambda take integer values. For the current value of the cosmological constant extended supergravities predict ultra light scalars with the mass of the order of Hubble constant, 10^{-33} eV. This may have interesting consequences for cosmology. Turning our attention to cosmological implications of M/string theory, we present a possibility to use string theory D-brane constructions to reproduce the main features of hybrid inflation. We stress an important role played by Fayet-Iliopoulos terms responsible for the positive contribution to the potentials and stabilization of moduli.

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引用

@article{arxiv.hep-th/0205315,
  title  = {Supergravity, M theory and Cosmology},
  author = {Renata Kallosh},
  journal= {arXiv preprint arXiv:hep-th/0205315},
  year   = {2007}
}

备注

24 pages, a talk at Stephen Hawking's 60th birthday conference, Cambridge University, Jan. 2002