Moduli Stabilisation versus Chirality for MSSM like Type IIB Orientifolds

Simple item page
dc.creatorBlumenhagen, Ralph
dc.creatorMoster, Sebastian
dc.creatorPlauschinn, Erik
dc.date2007-11-21
dc.date2007-12-14
dc.date.accessioned2026-07-07T11:13:20Z
dc.date.available2026-07-07T11:13:20Z
dc.descriptionWe 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.
dc.description43 pages, 4 figures, v2: refs. added
dc.identifierhttps://arxiv.org/abs/0711.3389
dc.identifierhttp://arxiv.org/abs/0711.3389
dc.identifierJHEP0801:058,2008
dc.identifierdoi:10.1088/1126-6708/2008/01/058
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191680
dc.subjectHigh Energy Physics - Theory
dc.subjectHigh Energy Physics - Phenomenology
dc.titleModuli Stabilisation versus Chirality for MSSM like Type IIB Orientifolds
dc.typetext

Files

Collections

arXiv