Dense geodesics, tower alignment, and the Sharpened Distance Conjecture

The Sharpened Distance Conjecture and Tower Scalar Weak Gravity Conjecture are closely related but distinct conjectures, neither one implying the other. Motivated by examples, I propose that both are consequences of two new conjectures: 1. The infinite distance geodesics passing through an arbitrary point phi in the moduli space populate a dense set of directions in the tangent space at phi. 2. Along any infinite distance geodesic, there exists a tower of particles whose scalar-charge-to-mass ratio (- backward difference log m) projection everywhere along the geodesic is greater than or equal to 1/d-2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ 1/\sqrt{d-2} $$\end{document}. I perform several nontrivial tests of these new conjectures in maximal and half-maximal supergravity examples. I also use the Tower Scalar Weak Gravity Conjecture to conjecture a sharp bound on exponentially heavy towers that accompany infinite distance limits.