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      A Simple No-Scale Model of Modulus Fixing and Inflation

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          Abstract

          We construct a no-scale model of inflation with a single modulus whose real and imaginary parts are both fixed by string-motivated corrections to the no-scale K{\" a}hler potential. Assuming an uplift of the minimum of the effective potential, the model yields a suitable number of e-folds of expansion and values of the tilt in the scalar cosmological density perturbations and of the ratio of tensor and scalar perturbations that are compatible with measurements of the cosmic microwave background radiation.

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          de Sitter Vacua in String Theory

          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 anti-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 10^10 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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            Two-loop self-energy diagrams with different masses and the momentum expansion

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              Yang-Mills theories with local supersymmetry: Lagrangian, transformation laws and super-Higgs effect

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                Author and article information

                Journal
                15 February 2018
                Article
                1802.05713
                cf4dbd43-9f7d-4fe1-a943-403821de8624

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                KCL-PH-TH/2018-05, CERN-PH-TH/2018-028
                12 pages, 6 figures
                hep-ph astro-ph.CO gr-qc hep-th

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