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Phys. Rev. D 68, 046005 (2003) [10 pages]

de Sitter vacua in string theory

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Shamit Kachru1,2, Renata Kallosh1, Andrei Linde1, and Sandip P. Trivedi3
1Department of Physics, Stanford University, Stanford, California 94305-4060, USA
2SLAC, Stanford University, Stanford, California 94309, USA
3TIFR, Homi Bhabha Road, Mumbai 400 005, India

Received 10 February 2003; published 7 August 2003

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 D3̅ -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 time scale of 1010yr. We also prove, under certain conditions, that the lifetime of dS space in string theory will always be shorter than the recurrence time.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.68.046005
DOI:
10.1103/PhysRevD.68.046005
PACS:
11.25.Yb, 98.80.-k