Moduli Self-Fixing

Abstract

In Quantum Gravity (QG), large moduli values lead to towers of exponentially light states, making the QG cut-off field-dependent. In 4D supersymmetric (SUSY) theories, this cut-off is set by the species scale $\Lambda(z_i, \bar{z}_i)$, where $z_i$ are complex moduli. We argue that in GKP-like 4D no-scale vacua, accounting for this field dependence generates one-loop, positive-definite potentials for the otherwise unfixed moduli, with local Minkowski minima at the desert points in moduli space with $z_i \sim \mathcal{O}(1)$. As these no-scale moduli grow, a dS plateau emerges and, for larger moduli, the potential runs away to zero, consistent with Swampland expectations. This may have important consequences for the moduli fixing problem. In particular non-perturbative superpotentials may not be necessary for fixing the K\"ahler moduli in a Type IIB setting. Although one loses control over non-perturbative corrections, we argue that modular invariance (more generally, dualities) of the species scale may give us information about the behaviour at small moduli in some simple cases. We illustrate this mechanism in a Type II 4D $\mathbb{Z}_2 \times \mathbb{Z}_2$ toroidal orientifold, where in some cases, modular invariance can give us control over the non-perturbative corrections. The vanishing cosmological constant reflects a delicate cancellation between IR and UV contributions at the minimum. The models may be completed by the addition of intersecting D6-branes, yielding a 3-generation MSSM (RR tadpole free) model with some (but not all) closed string moduli fixed in Minkowski, with the complex structure moduli fixed at the desert points.