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Constraints on Lorentz-invariance violation in the neutrino sector from the ultrahigh-energy event KM3-230213A

Yu-Ming Yang ^1,2,*, Xing-Jian Lv ^1,2,†, Xiao-Jun Bi ^1,2,‡, and Peng-Fei Yin ^1,§

¹State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
²School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China

^*Contact author: yangyuming@ihep.ac.cn
^†Contact author: lvxj@ihep.ac.cn
^‡Contact author: bixj@ihep.ac.cn
^§Contact author: yinpf@ihep.ac.cn

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A possible cosmological origin of the KM3-230213A event

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Articles Citing

Constraints on Lorentz-invariance violation in the neutrino sector from the ultrahigh-energy event KM3-230213A

Could a Primordial Black Hole Explosion Explain the Extremely High-Energy KM3NeT Neutrino Event?

Tackling transient sources with neutrino telescopes

Implications of the KM3NeT ultrahigh-energy event on neutrino self-interactions

Neutrino transition dipole moments in light of the KM3NeT event

Probing Lorentz invariance violation in cosmogenic neutrino propagation with KM3-230213A

No flavor anisotropy in the high-energy neutrino sky upholds Lorentz invariance

Ultra-High-Energy Tau Neutrinos as Probes of Lorentz Invariance

Superluminal constraints from ultra-high-energy neutrino events

Vector-field spontaneous baryogenesis with Lorentz invariance violation

What KM3-230213A event may tell us about the neutrino mass and dark matter

Super heavy dark matter origin of the PeV neutrino event: KM3-230213A

Looking for the gamma-Ray cascades of the KM3-230213A neutrino source

A possible cosmological origin of the KM3-230213A event

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