Key points are not available for this paper at this time.
A cosmic axion, via the electromagnetic anomaly, induces an oscillating electric dipole for the electron of frequency m₀ and strength (few) 10^-32 e-cm, two orders of magnitude above the nucleon, and within a few orders of magnitude of the present standard model constant limit. We give a detailed study of this phenomenon via the interaction of the cosmic axion, through the electromagnetic anomaly, with particular emphasis on the decoupling limit of the axion, ₓa (t) m₀0. The analysis is subtle, and we find the general form of the action involves a local contact interaction and a nonlocal contribution, analogous to the ``transverse current'' in QED, that enforces the decoupling limit. We carefully derive the effective action in the Pauli-Schr\"odinger nonrelativistic formalism, and in Georgi's heavy quark formalism adapted to the ``heavy electron'' (m₄m₀). We compute the electric dipole radiation emitted by free electrons, magnets and currents, immersed in the cosmic axion field, and discuss experimental configurations that may yield a detectable signal.
Christopher T. Hill (Tue,) studied this question.