Articles Citing

Possible origin of the KM3-230213A neutrino event from dark matter decay

Debasish Borah ^1,2,*, Nayan Das ^1,†, Nobuchika Okada ^3,‡, and Prantik Sarmah ^4,§

¹Department of Physics, Indian Institute of Technology Guwahati, Assam 781039, India
²Pittsburgh Particle Physics, Astrophysics, and Cosmology Center, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA
³Department of Physics, University of Alabama, Tuscaloosa, Alabama 35487, USA
⁴Institute of High Energy PhysicsChinese Academy of Sciences, Beijing 100049, People’s Republic of China

^*Contact author: dborah@iitg.ac.in
^†Contact author: nayan.das@iitg.ac.in
^‡Contact author: okadan@ua.edu
^§Contact author: prantiksarmah@ihep.ac.cn

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Articles Citing

Possible origin of the KM3-230213A neutrino event from dark matter decay

Dark matter

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

Hunting heavy decaying dark matter with Tibet ASγ and LHAASO-KM2A

Tackling transient sources with neutrino telescopes

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

Constraining superheavy dark matter with the KM3-230213A neutrino event

Neutrino transition dipole moments in light of the KM3NeT event

Neutron portal to ultrahigh-energy neutrinos

KM3-230213A and IceCube neutrino events from metastable dark matter of primordial black hole origin

Highest-energy neutrino event constrains dark matter-neutrino interactions

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

Ultra-High Energy Event KM3-230213A as a Cosmogenic Neutrino in Light of Minimal UHECR Flux Models

Exploring ultra-high energy neutrino experiments through the lens of the transport equation

Seafloor topography enhances KM3NeT sensitivity to ANITA-like events

Superluminal constraints from ultra-high-energy neutrino events

Explaining the KM3-230213A detection without gamma-ray emission: cosmic-ray dark radiation

LHAASO galactic plane γ-rays strongly constrain heavy dark matter

Decaying vector dark matter with low reheating temperature for KM3NeT signal and its impact on gravitational waves

Probing super-heavy dark matter with ultra-high-energy gamma rays

KM3NeT 220 PeV event: A neutrino messenger from the grand unification scale?

Implications of a Cosmogenic Origin of KM3-230213A for Ultra-high-energy Protons

Galaxy Clusters in Dark Matter Window: The Case of the Shapley Supercluster

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

Ultrahigh-energy neutrino event KM3-230213A as a signal of electroweak vacuum turbulence in merging black hole binaries

Superheavy supersymmetric dark matter as the origin of the KM3NeT ultrahigh energy signal

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