Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published December 2014 | Submitted + Published
Journal Article Open

Infrared Consistency and the Weak Gravity Conjecture

Abstract

The weak gravity conjecture (WGC) asserts that an Abelian gauge theory coupled to gravity is inconsistent unless it contains a particle of charge q and mass m such that q≥m/m_(Pl). This criterion is obeyed by all known ultraviolet completions and is needed to evade pathologies from stable black hole remnants. In this paper, we explore the WGC from the perspective of low-energy effective field theory. Below the charged particle threshold, the effective action describes a photon and graviton interacting via higher-dimension operators. We derive infrared consistency conditions on the parameters of the effective action using i ) analyticity of light-by-light scattering, ii ) unitarity of the dynamics of an arbitrary ultraviolet completion, and iii ) absence of superluminality and causality violation in certain non-trivial backgrounds. For convenience, we begin our analysis in three spacetime dimensions, where gravity is non-dynamical but has a physical effect on photon-photon interactions. We then consider four dimensions, where propagating gravity substantially complicates all of our arguments, but bounds can still be derived. Operators in the effective action arise from two types of diagrams: those that involve electromagnetic interactions (parameterized by a charge-to-mass ratio q/m) and those that do not (parameterized by a coefficient γ). Infrared consistency implies that q/m is bounded from below for small γ.

Additional Information

© 2014 The Author(s). This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. Article funded by SCOAP3. Received: August 30, 2014; Accepted: November 21, 2014; Published: December 11, 2014. We thank Allan Adams, Nima Arkani-Hamed, Brando Bellazzini, Sean Carroll, Stanley Deser, Tim Hollowood, Stefan Leichenauer, Alberto Nicolis, Rafael Porto, and Ira Rothstein for useful discussions and comments. C.C. is supported by a Sloan Research Fellowship and a DOE Early Career Award under Grant No. DE-SC0010255. G.N.R. is supported by a Hertz Graduate Fellowship and a NSF Graduate Research Fellowship under Grant No. DGE-1144469.

Attached Files

Published - art_3A10.1007_2FJHEP12_282014_29087.pdf

Submitted - 1407.7865v1.pdf

Files

1407.7865v1.pdf
Files (1.7 MB)
Name Size Download all
md5:a97ba10e10795a88b1b700f8ee0504cf
839.5 kB Preview Download
md5:54b34d9996b43cab179d88cfc7cee81e
856.5 kB Preview Download

Additional details

Created:
August 20, 2023
Modified:
February 10, 2024