A Weak Gravity Theorem
Abstract
In a gravitational theory with a massless photon the maximum charge-to-mass ratio of black holes approaches the prediction of the Einstein-Maxwell theory as black hole mass increases: for some constant . We will show that if below the quantum gravity scale there are many degrees of freedom with a hierarchically small mass gap . In this regime one can treat gravity as a non-dynamical background field and derive field-theoretic sum-rules for the coefficients of the leading corrections to the Einstein-Maxwell theory. The positivity of follows from the sum-rules. As a consequence, gravitational attraction gets weaker than the electric force among maximally charged black holes as they become lighter, and large extremal black holes can decay into smaller black holes.
Cite
@article{arxiv.1905.02736,
title = {A Weak Gravity Theorem},
author = {Mehrdad Mirbabayi},
journal= {arXiv preprint arXiv:1905.02736},
year = {2019}
}
Comments
Withdrawn because the assumptions made in sections 2.1 and 3.1 about the UV coefficients can be justified only when $g M_{pl} \sim \Lambda$. Therefore the assumption (ii) of section 1.1 is effectively assuming the existence of QFT states with parametrically large charge-to-mass ratio