Model Building and Phenomenology of Flux-Induced Supersymmetry Breaking on D3-branes
Fernando Marchesano, Gary Shiu, Lian-Tao Wang
TL;DR
The paper provides a concrete string-theoretic realization of flux-induced supersymmetry breaking on D3-branes at singularities, demonstrating how NSNS and RR 3-form fluxes generate both soft SUSY-breaking terms and a mu-term in locally chiral models and embedding them into global flux compactifications. By constructing a local ${f Z}_4$ model and a global ${f Z}_4$ flux vacuum, it shows that the low-energy spectrum can resemble MSSM features and that the soft parameters are dictated by the background flux, yielding a dilaton-dominated-like pattern with universal soft terms. A key phenomenological insight is that flux quantization ties the mu-term and soft masses together, which can alter the conventional electroweak fine-tuning expectations; depending on Kähler moduli stabilization, the tuning with respect to the soft scale may be linear, constant, or even more favorable in higher-scale scenarios. The analysis highlights how global consistency conditions, flux quantization, and NSNS tadpoles shape viable vacua and their electroweak phenomenology, offering a framework for exploring more realistic flux vacua and their collider/cosmological implications.
Abstract
We study supersymmetry breaking effects induced on D3-branes at singularities by the presence of NSNS and RR 3-form fluxes. First, we discuss some local constructions of chiral models from D3-branes at singularities, as well as their global embedding in flux compactifications. The low energy spectrum of these constructions contains features of the supersymmetric Standard Model. In these models, both the soft SUSY parameters and the mu-term are generated by turning on the 3-form NSNS and RR fluxes. We then explore some model-independent phenomenological features as, e.g., the fine-tuning problem of electroweak symmetry breaking in flux compactifications. We also comment on other phenomenological features of this scenario.
