For a neutron star with a 10^17 G central field and a 15 meV axion, the paper predicts that magnetic fields raise axion luminosity and reshape the axion-to-photon flux, with bremsstrahlung dominating at low axion energies.
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QCD Axion Conversion in Magnetospheres of Neutron Stars
For a neutron star with a 10^17 G central field and a 15 meV axion, the paper predicts that magnetic fields raise axion luminosity and reshape the axion-to-photon flux, with bremsstrahlung dominating at low axion energies.