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.

Highlights

  • The power of the Weak Gravity Conjecture (WGC) lies in its generality

  • 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 explore the constraints posed by modular invariance on a particular discrete ZN symmetry which arises in our discussion

Read more

Summary

Gravity and gauge fields in three dimensions

There are qualitative differences in the physics of both gravity and matter between three and more spacetime dimensions. [39] gives a clear exposition of the peculiarities of gravity in the 3d case. The total electrostatic energy of a particle is IR divergent, as well as UV divergent This already signals trouble with charged particles and gravity: the backreaction of a point particle on the geometry is significant, in the same way as for strings charged under a B-field in four dimensions or D7-branes in type II string theory [40, 41]. No free charged particles are present in the theory (the low energy dynamics of the gauge field is that of a scalar field with a cosine potential). There is another possibility which solves the problem: in three dimensions,one can give a topological gauge-invariant mass to the U(1) via a Chern-Simons term.

Consequences of compactness of the gauge group
Black hole solutions
Black hole discharge in AdS
Extended chiral algebra and the Sugawara construction
An extremality bound
Modular invariance
Constraints on theories with level N current algebras
Modular invariance constraints
An example based on alignment
Modular bootstrap approach
Conclusions
A Duality between Chern-Simons and current algebra
B Constraints on the partition function from modular invariance
Spectral flow from modular invariance
Cardy’s formula for the charge Q sector
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call