English

A Weak Gravity Theorem

High Energy Physics - Theory 2019-07-09 v3 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

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: Qext/M=1+α/M2Q_{\rm ext}/M =1+ \alpha/M^2 for some constant α\alpha. We will show that α>0\alpha>0 if below the quantum gravity scale Λ\Lambda there are many degrees of freedom with a hierarchically small mass gap log(Λ/mgap)1\log(\Lambda/m_{\rm gap})\gg 1. 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 α\alpha 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.

Keywords

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Withdrawn because the assumptions made in sections 2.1 and 3.1 about the UV coefficients can be justified only when $g M_{pl} \sim \Lambda$.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