Detection of the 220 PeV neutrino KM3-230213A implies that superluminal Lorentz violation in the neutrino sector must have a mass scale above 1.1x10^30 GeV (n=1) or 1.1x10^19 GeV (n=2), assuming the event originated extragalactically.
Constraints on Neutrino Velocities Revisited
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abstract
With a minimally modified dispersion relation for neutrinos, we reconsider the constraints on superluminal neutrino velocities from bremsstrahlung effects in the laboratory frame. Employing both the direct calculation approach and the virtual Z-boson approach, we obtain the generic decay width and energy loss rate of a superluminal neutrino with general energy. The Cohen-Glashow's analytical results for neutrinos with a relatively low energy are confirmed in both approaches. We employ the survival probability instead of the terminal energy to assess whether a neutrino with a given energy is observable or not in the OPERA experiment. Moreover, using our general results we perform systematical analyses on the constraints arising from the Super-Kamiokande and IceCube experiments.
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Ultra-high-energy event KM3-230213A constraints on Lorentz Invariance Violation in neutrino sector
Detection of the 220 PeV neutrino KM3-230213A implies that superluminal Lorentz violation in the neutrino sector must have a mass scale above 1.1x10^30 GeV (n=1) or 1.1x10^19 GeV (n=2), assuming the event originated extragalactically.