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Gravity-induced photon interactions and infrared consistency in any dimensions

Pedro Bittar1,*, Sylvain Fichet2,†, and Lucas de Souza3,‡

  • *Contact author: pedro.bittar.souza@usp.br
  • †Contact author: sylvain.fichet@ufabc.edu.br
  • ‡Contact author: souza.l@ufabc.edu.br

Phys. Rev. D 112, 045009 – Published 21 August, 2025

DOI: https://doi.org/10.1103/p8k8-vz2h

Abstract

We compute the four-photon (F4) operators generated by loops of charged particles of spin 0, 12, 1 in the presence of gravity and in any spacetime dimension d. To this end, we expand the one-loop effective action via the heat kernel coefficients, which capture both the gravity-induced renormalization of the F4 operators and the low-energy Einstein-Maxwell effective field theory (EFT) produced by massive charged particles. We set positivity bounds on the F4 operators using standard arguments from extremal black holes (for d≥4) and from infrared (IR) consistency of four-photon scattering (for d≥3). We find that both approaches yield nearly equivalent results, even though in the amplitudes we discard the graviton t-channel pole and use the vanishing of the Gauss-Bonnet term at quadratic order for any d. The positivity bounds constrain the charge-to-mass ratio of the heavy particles. If the Planckian F4 operators are sufficiently small or negative, such bounds produce a version of the d-dimensional weak gravity conjecture (WGC) in most, but not all, dimensions. In the special case of d=6, the gravity-induced beta functions of F4 operators from charged particles of any spin are positive, leading to WGC-like bounds with a logarithmic enhancement. In d=9, 10, the WGC fails to guarantee extremal black hole decay in the infrared EFT, thereby requiring the existence of sufficiently large Planckian F4 operators.

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