Lorentz-violating photons can decay to neutrino pairs via the SM anapole vertex; the rate is too weak for stronger bounds except when electron-pair decay is kinematically closed.
Constraining Superluminal Electron and Neu- trino Velocities using the 2010 Crab Nebula Flare and the Ice- Cube PeV Neutrino Events
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Lorentz-Violating Photon Decay into Neutrinos and Constraints from PeV Photon Stability
Lorentz-violating photons can decay to neutrino pairs via the SM anapole vertex; the rate is too weak for stronger bounds except when electron-pair decay is kinematically closed.