Type IIB Supersymmetric Flux Vacua
Ching-Ming Chen, Shan Hu, Tianjun Li, Dimitri V. Nanopoulos

TL;DR
This paper investigates supersymmetric flux vacua in Type IIB string theory on toroidal orientifolds, revealing constraints on flux contributions and tadpole cancellation, and constructing semi-realistic models with relaxed tadpole conditions.
Contribution
It demonstrates the impossibility of simultaneously having positive moduli and negative flux contributions in Minkowski vacua, and constructs semi-realistic AdS models with relaxed tadpole conditions.
Findings
Positive flux contributions are necessary for stabilized Minkowski vacua.
Relaxed tadpole conditions are achievable in AdS vacua but not in Minkowski vacua.
Constructed a semi-realistic Pati-Salam model from flux compactifications.
Abstract
On the Type IIB toroidal T^6 orientifolds with generic flux compactifications, we conjecture that in generic supsersymmetric Minkowski vacua, at least one of the flux contributions to the seven-brane and D3-brane tadpoles is positive if the moduli are stabilized properly, and then the tadpole cancellation conditions can not be relaxed. To study the supsersymmetric Minkowski flux vacua, we simplify the fluxes reasonably and discuss the corresponding superpotential. We show that we can not have simultaneously the positive real parts of all the moduli and the negative/zero flux contributions to all the seven-brane and D3-brane tadpoles. Therefore, we can not construct realistic flux models with the relaxed tadpole cancellation conditions. When studying the supsersymmetric AdS vacua, we obtain flux models with the seven-brane and D3-brane tadpole cancellation conditions relaxed elegantly,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Pulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations
