Using a recently developed effective field theory formalism for extreme mass
ratios [2308.14832], we present a calculation of charged black hole scattering
at third post-Minkowskian order. The charges and masses are kept arbitrary, and
the result interpolates from the scattering of Schwarzschild to extremal
charged black holes, and beyond to charged particles in electrodynamics --
agreeing with previously reported results in all such limits. The computation
of the radial action is neatly organized in powers of the mass ratio. The probe
(0SF) contributions are readily computed by direct integration of the radial
momentum, and we use the effective field theory to compute the subleading (1SF)
contributions via background-field Feynman rules supplemented by an operator
encoding recoil of the background. Together these contributions completely
determine the conservative physics at order~O(G3).Comment: 36 pages, 3 figure