de Sitter vacua in string theory
Shamit Kachru A, Рената Каллош, Andrei D Linde, Sandip P. Trivedi
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 2003 · 3,345 citationsOpen access
Abstract
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 $\overline{\mathrm{D}3}$-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 ${10}^{10}\mathrm{yr}.$ We also prove, under certain conditions, that the lifetime of dS space in string theory will always be shorter than the recurrence time.
Cite this paper
A, S. K., Каллош, Р., Linde, A. D., & Trivedi, S. P. (2003). de sitter vacua in string theory. Physical Review. D. Particles, Fields, Gravitation, and Cosmology Physical Review. D. Particles and Fields, 68(4). https://doi.org/10.1103/physrevd.68.046005
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