The Convex Hull Swampland Distance Conjecture and Bounds on Non-geodesics

TL;DR

This paper explores how the Swampland Distance Conjecture constrains non-geodesic trajectories in moduli space, introducing a convex hull framework and analyzing implications for string theory flux compactifications.

Contribution

It introduces a convex hull formulation of the SDC for trajectories with scalar potentials, extending understanding of non-geodesic limits in string theory.

Findings

Critical trajectories for maximum non-geodesicity identified.

Convex hull constraint on scalar charge-to-mass ratios established.

Flux compactifications realize these critical non-geodesic behaviors.

Abstract

The Swampland Distance Conjecture (SDC) restricts the geodesic distances that scalars can traverse in effective field theories as they approach points at infinite distance in moduli space. We propose that, when applied to the subset of light fields in effective theories with scalar potentials, the SDC restricts the amount of non-geodesicity allowed for trajectories along valleys of the potential. This is necessary to ensure consistency of the SDC as a valid swampland criterium at any energy scale across the RG flow. We provide a simple description of this effect in moduli space of hyperbolic space type, and products thereof, and obtain critical trajectories which lead to maximum non-geodesicity compatible with the SDC. We recover and generalize these results by expressing the SDC as a new Convex Hull constraint on trajectories, characterizing towers by their scalar charge to mass ratio in analogy to the Scalar Weak Gravity Conjecture. We show that recent results on the asymptotic scalar potential of flux compatifications near infinity in moduli space precisely realize these critical amounts of non-geodesicity. Our results suggest that string theory flux compactifications lead to the most generic potentials allowing for maximum non-geodesicity of the potential valleys while respecting the SDC along them.