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Sequestered de Sitter string scenarios: soft-terms

2014/09/05 by Luis Aparicio, Michele Cicoli, Sven Krippendorf +3 · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #De Sitter universe #Gaugino #Gravitino #Moduli #Particle physics theoretical and experimental studies #String (physics) #String theory #Supersymmetry #Supersymmetry breaking #hep-ph #hep-th

paper · pdf · doi:10.1007/jhep11(2014)071

27 pages + appendices, 2 figures

arxiv created 2014/09/05 · openalex publication_date 2014/11/01 · arxiv updated 2015/06/22 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We analyse soft supersymmetry breaking in type IIB de Sitter string vacua after moduli stabilisation, focussing on models in which the Standard Model is sequestered from the supersymmetry breaking sources and the spectrum of soft-terms is hierarchically smaller than the gravitino mass m 3/2. Due to this feature, these models are compatible with gauge coupling unification and TeV scale supersymmetry with no cosmological moduli problem. We determine the influence on soft-terms of concrete realisations of de Sitter vacua constructed from supersymmetric effective actions. One of these scenarios provides the first study of soft-terms for consistent string models embedded in a compact Calabi-Yau manifold with all moduli stabilised. Depending on the moduli dependence of the Kähler metric for matter fields and on the mechanism responsible to obtain a de Sitter vacuum, we find two scenarios for phenomenology: (i) a split-supersymmetry scenario where gaugino masses are suppressed with respect to scalar masses: M 1/2 ∼ m 3/2 ϵ ≪ m 0 ∼ m 3/2 √(ε ) ≪ m 3/2 for ϵ ∼ m 3/2 /M P ≪ 1; (ii) a typical MSSM scenario where all soft-terms are of the same order: M 1/2 ∼ m 0 ∼ m 3/2 ϵ ≪ m 3/2. Background fluxes determine the numerical coefficients of the soft-terms allowing for small variations of parameters as is necessary to confront data and to interpolate between different scenarios. We comment on different stringy origins of the μ-term and potential sources of desequestering.

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