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The Weak Gravity Conjecture in three dimensions

Miguel Montero, Gary Shiu, Pablo Soler

TL;DR

This work analyzes the Weak Gravity Conjecture in AdS$_3$ with a weakly coupled U(1) gauge field, showing that modular invariance of the holographic CFT together with gauge-compactness implies the existence of light charged operators below the charged BTZ black hole threshold, realizing a 3D version of the WGC. The authors derive this from the Sugawara decomposition of the stress tensor and the spectral-flow automorphism, which together guarantee light, charged primaries in appropriate sectors. They also study discrete $ ext{Z}_N$ charges, demonstrating that modular invariance alone does not guarantee light $ ext{Z}_N$-charged states and providing a concrete lattice example where the lowest charged state can be arbitrarily heavy. Additionally, a modular bootstrap approach is developed to bound charged operator dimensions in $ ext{Z}_N$ sectors, revealing nontrivial constraints for small $N$ but no universal bound for larger $N$. Overall, the paper argues that modular invariance and current-algebra structure imply a form of the WGC in three dimensions, while highlighting important distinctions from higher-dimensional remnants arguments and from discrete-charge sectors.

Abstract

We study weakly coupled $U(1)$ theories in $AdS_3$, their associated charged BTZ solutions, and their charged spectra. We find that modular invariance of the holographic dual two-dimensional CFT and compactness of the gauge group together imply the existence of charged operators with conformal dimension significantly below the black hole threshold. We regard this as a form of the Weak Gravity Conjecture (WGC) in three dimensions. We also explore the constraints posed by modular invariance on a particular discrete $\mathbb{Z}_N$ symmetry which arises in our discussion. In this case, modular invariance does not guarantee the existence of light $\mathbb{Z}_N$-charged states. We also highlight the differences between our discussion and the usual heuristic arguments for the WGC based on black hole remnants.

The Weak Gravity Conjecture in three dimensions

TL;DR

This work analyzes the Weak Gravity Conjecture in AdS with a weakly coupled U(1) gauge field, showing that modular invariance of the holographic CFT together with gauge-compactness implies the existence of light charged operators below the charged BTZ black hole threshold, realizing a 3D version of the WGC. The authors derive this from the Sugawara decomposition of the stress tensor and the spectral-flow automorphism, which together guarantee light, charged primaries in appropriate sectors. They also study discrete charges, demonstrating that modular invariance alone does not guarantee light -charged states and providing a concrete lattice example where the lowest charged state can be arbitrarily heavy. Additionally, a modular bootstrap approach is developed to bound charged operator dimensions in sectors, revealing nontrivial constraints for small but no universal bound for larger . Overall, the paper argues that modular invariance and current-algebra structure imply a form of the WGC in three dimensions, while highlighting important distinctions from higher-dimensional remnants arguments and from discrete-charge sectors.

Abstract

We study weakly coupled theories in , their associated charged BTZ solutions, and their charged spectra. We find that modular invariance of the holographic dual two-dimensional CFT and compactness of the gauge group together imply the existence of charged operators with conformal dimension significantly below the black hole threshold. We regard this as a form of the Weak Gravity Conjecture (WGC) in three dimensions. We also explore the constraints posed by modular invariance on a particular discrete symmetry which arises in our discussion. In this case, modular invariance does not guarantee the existence of light -charged states. We also highlight the differences between our discussion and the usual heuristic arguments for the WGC based on black hole remnants.

Paper Structure

This paper contains 24 sections, 91 equations.