Chiral 4d string vacua with D-branes and NSNS and RR fluxes
Juan F. G. Cascales, Angel M. Uranga
TL;DR
This work constructs chiral four-dimensional string vacua by combining D-branes with NSNS and RR 3-form fluxes in type IIB orientifolds, using magnetised D9-branes on $T^6/(\mathbb{Z}_2\times\mathbb{Z}_2)$ to generate chiral spectra while stabilizing most moduli through fluxes. The authors analyze consistency conditions, SUSY preservation, and anomaly cancellation, providing explicit models with supersymmetric subsectors and even a non-supersymmetric SU(5) example, all while ensuring RR tadpole cancellation. A key insight is that fluxes stabilize complex structure and many Kahler moduli, and the magnetised-brane setup yields tractable chiral spectra; the framework also maps, under T-duality, to D8-branes on non-Calabi-Yau half-flat geometries with metric fluxes. Discrete B-fields and dual descriptions further enrich model-building options, including RR-tadpole reshaping and new Wess-Zumino couplings, suggesting a versatile path toward realistic string vacua with stabilized moduli and chiral matter.
Abstract
We discuss type IIB orientifolds with D-branes, and NSNS and RR field strength fluxes. The D-brane sectors lead to open string spectra with non-abelian gauge symmetry and charged chiral fermions. The closed string field strengths generate a scalar potential stabilizing most moduli. We describe the construction of N=1 supersymmetric models in the context of orientifolds of IIB theory on T^6/Z_2 x Z_2, containing D9-branes with world-volume magnetic fluxes, and illustrate model building possibilities with several explicit examples. We comment on a T-dual picture with D8-branes on non-Calabi-Yau half-flat geometries, and discuss some of the topological properties of such configurations. We also explore the construction of models with fluxes and with D3-branes at singularities and present a non-supersymmetric 3-family SU(5) model.
