Answers are grounded in this paper and cite their sources.
We propose new physical processes based on the axial vector anomaly and described by the Wess-Zumino-Witten term that couples the photon, Z-boson, and the ω-meson. The interaction takes the form of a pseudo-Chern-Simons term, ~ϵ_μνρσω^μZ^νF^ρσ. This term induces neutrino-photon interactions at finite baryon density via the coupling of the Z-boson to neutrinos. These interactions may be detectable in various laboratory and astrophysical arenas. The new interactions may account for the excess observed at the Fermilab Booster Neutrino Experiment MiniBooNE. They also produce a competitive contribution to neutron star cooling at temperatures 10⁹ K. These processes and related axion-photon interactions at finite baryon density appear to be relevant in many astrophysical regimes.
No takes yet. Share an insight, caveat, or question.
Harvey et al. (2007) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: