2007
DOI: 10.1103/physrevd.75.025019
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Moduli stabilization,F-term uplifting, and soft supersymmetry breaking terms

Abstract: We study moduli stabilization with F-term uplifting. As a source of uplifting F-term, we consider spontaneous supersymmetry breaking models, e.g. the Polonyi model and the Intriligator-Seiberg-Shih model. We analyze potential minima by requiring almost vanishing vacuum energy and evaluate the size of modulus F-term. We also study soft SUSY breaking terms. In our scenario, the mirage mediation is dominant in gaugino masses. Scalar masses can be comparable with gaugino masses or much heavier, depending on coupli… Show more

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Cited by 142 publications
(151 citation statements)
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“…35 We have again made a convenient choice for the integration constant in s. 36 More generally, a holomorphic 1-form on a genus g curve of this type will have g free parameters, which is enough freedom to fix the A-periods but further imposing constraints on B-periods fixes the moduli. On the other hand, a harmonic 1-form on a genus g curve of this type will have 2g free parameters, which is enough freedom to fix all periods for arbitrary values of the moduli.…”
Section: First Attempts At An M-theory Liftmentioning
confidence: 99%
See 1 more Smart Citation
“…35 We have again made a convenient choice for the integration constant in s. 36 More generally, a holomorphic 1-form on a genus g curve of this type will have g free parameters, which is enough freedom to fix the A-periods but further imposing constraints on B-periods fixes the moduli. On the other hand, a harmonic 1-form on a genus g curve of this type will have 2g free parameters, which is enough freedom to fix all periods for arbitrary values of the moduli.…”
Section: First Attempts At An M-theory Liftmentioning
confidence: 99%
“…Because such configurations do not correspond to true vacua, many of the difficulties associated with the construction of realistic models of supersymmetry-breaking can be avoided. As such, the ideas of [1] have already found wide phenomenological application [33,34,35,36,37,38,39,40,41].…”
Section: Introductionmentioning
confidence: 99%
“…There, the scalar potential is well approximated by 9) where V ISS is the global supersymmetric (as opposed to supergravity) scalar potential for the ISS sector. However, when computing the critical temperature, we will consider the expansion (2.9) to be valid at the origin of the field space as well.…”
Section: Iss-kklt Modelmentioning
confidence: 99%
“…However, due to their large masses, the high temperature expansion can not be used. From (3.3), we derive a low temperature expansion 9) with M B, F ≫ Θ. At the leading order, the squarks mass matrix is almost diagonal and its eigenvalues are h 2 Φ 2 / T 0 + T 0 3 .…”
Section: Formation Of the Supersymmetric Vacuamentioning
confidence: 99%
“…Note that ln (M p /m 3/2 ) ∼ O 8π 2 and compensate the loop suppression factors appeared in the anomaly mediated contributions. α = 1 is realized in the original KKLT-setup [28], but various rational values can be obtained in the similar setups [8,9,29,30]. An important fact is that α could be determined by rational parameters, such as the winding number of D-branes and the number of fluxes which generates moduli potential.…”
Section: Jhep11(2017)189mentioning
confidence: 99%