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.
Squeezing the Parameter Space for Lorentz Violation in the Neutrino Sector by Additional Decay Channels
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abstract
The hypothesis of Lorentz violation in the neutrino sector has intrigued scientists for the last two to three decades. A number of theoretical arguments support the emergence of such violations first and foremost for neutrinos, which constitute the "most elusive" and "least interacting" particles known to mankind. It is of obvious interest to place stringent bounds on the Lorentz-violating parameters in the neutrino sector. In the past, the most stringent bounds have been placed by calculating the probability of neutrino decay into a lepton pair, a process made kinematically feasible by Lorentz violation in the neutrino sector, above a certain threshold. However, even more stringent bounds can be placed on the Lorentz-violating parameters if one takes into account, additionally, the possibility of neutrino splitting, i.e., of neutrino decay into a neutrino of lower energy, accompanied by "neutrino-pair Cerenkov radiation". This process has negligible threshold and can be used to improve the bounds on Lorentz-violating parameters in the neutrino sector. Finally, we take the opportunity to discuss the relation of Lorentz and gauge symmetry breaking, with a special emphasis on the theoretical models employed in our calculations.
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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.