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De Sitter Vacua in String Theory
Open accessAbstract
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 {ovr 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{sup 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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Beyond the cosmological standard model
Joyce, A., Jain, B., Khoury, J., & Trodden, M. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.12.002 · Cited by 1,231
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The best inflationary models after Planck
Martin, J., Ringeval, C., Trotta, R., & Vennin, V. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/03/039 · Cited by 301
The anthropic landscape of string theory
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Metadata
- Authors
- Kachru, S.
- Published
- 2003-02-28
- OpenAlex
- W4206678947
- Cited by
- 361
- References
- 51
- Type
- report
- Language
- en
- Open access
- green
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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