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Moduli Stabilisation versus Chirality for MSSM like Type IIB Orientifolds

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arxiv 0711.3389 v2 pith:GUQAYA5V submitted 2007-11-21 hep-th hep-ph

Ralph Blumenhagen , Sebastian Moster , Erik Plauschinn This is my paper · ORCID
classification hep-thhep-ph
keywords modulistabilisationtypechiralf-termslargelikemssm
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We investigate the general question of implementing a chiral MSSM like D-brane sector in Type IIB orientifold models with complete moduli stabilisation via F-terms induced by fluxes and space-time instantons, respectively gaugino condensates. The prototype examples are the KKLT and the so-called large volume compactifications. We show that the ansatz of first stabilising all moduli via F-terms and then introducing the Standard Model module is misleading, as a chiral sector notoriously influences the structure of non-perturbative effects and induces a D-term potential. Focusing for concreteness on the large volume scenario, we work out the geometry of the swiss-cheese type Calabi-Yau manifold P_[1,3,3,3,5][15]_(3,75) and analyse whether controllable and phenomenologically acceptable Kaehler moduli stabilisation can occur by the combination of F- and D-terms.

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Cited by 4 Pith papers

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