de Sitter vacua in string theory
- 1. SLAC, Stanford University, Stanford, California 94309 (United States)
- 2. Department of Physics, Stanford University, Stanford, California 94305-4060 (United States)
- 3. TIFR, Homi Bhabha Road, Mumbai 400 005 (India)
Description
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 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 time scale of 1010 yr. We also prove, under certain conditions, that the lifetime of dS space in string theory will always be shorter than the recurrence time
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.68.046005;
- arXiv
- arXiv:hep-th/0301240v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 68
- Journal Issue
- 4
- Journal Page Range
- p. 046005-046005.10
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35082210
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COMPACTIFICATION; CORRECTIONS; GEOMETRY; GROUND STATES; INSTANTONS; LIFETIME; MEMBRANES; POTENTIALS; QUANTUM FIELD THEORY; SMOOTH MANIFOLDS; SPACE-TIME; SPARTICLES; SUPERSTRING MODELS; SUPERSYMMETRY
- Descriptors DEC
- COMPOSITE MODELS; ELEMENTARY PARTICLES; ENERGY LEVELS; EXTENDED PARTICLE MODEL; FIELD THEORIES; MATHEMATICAL MANIFOLDS; MATHEMATICAL MODELS; MATHEMATICS; PARTICLE MODELS; POSTULATED PARTICLES; QUARK MODEL; QUASI PARTICLES; STRING MODELS; SYMMETRY
Optional Information
- Notes
- (c) 2003 The American Physical Society