- Open Access
Gravity-induced photon interactions and infrared consistency in any dimensions
Phys. Rev. D 112, 045009 – Published 21 August, 2025
DOI: https://doi.org/10.1103/p8k8-vz2h
Abstract
We compute the four-photon () operators generated by loops of charged particles of spin 0, , 1 in the presence of gravity and in any spacetime dimension . To this end, we expand the one-loop effective action via the heat kernel coefficients, which capture both the gravity-induced renormalization of the operators and the low-energy Einstein-Maxwell effective field theory (EFT) produced by massive charged particles. We set positivity bounds on the operators using standard arguments from extremal black holes (for ) and from infrared (IR) consistency of four-photon scattering (for ). We find that both approaches yield nearly equivalent results, even though in the amplitudes we discard the graviton -channel pole and use the vanishing of the Gauss-Bonnet term at quadratic order for any . The positivity bounds constrain the charge-to-mass ratio of the heavy particles. If the Planckian operators are sufficiently small or negative, such bounds produce a version of the -dimensional weak gravity conjecture (WGC) in most, but not all, dimensions. In the special case of , the gravity-induced beta functions of operators from charged particles of any spin are positive, leading to WGC-like bounds with a logarithmic enhancement. In , 10, the WGC fails to guarantee extremal black hole decay in the infrared EFT, thereby requiring the existence of sufficiently large Planckian operators.
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