Super heavy dark matter origin of the PeV neutrino event: KM3-230213A
arXiv:2503.04464 · doi:10.1103/vvqq-1z2t
Abstract
The recent observation of the ultrahigh-energy neutrino event KM3-230213A by the KM3NeT experiment offers a compelling avenue to explore physics beyond the Standard Model (SM). In this paper, we explore a simplest possibility that this event originates from the decay of a super-heavy dark matter (SHDM). We consider a minimal scenario where the SHDM decays to neutrino and SM Higgs. We derive constraints on the DM lifetime as a function of DM mass, ensuring consistency with IceCube, Auger upper limits, and the observed KM3-230213A event, along with the gamma-ray constraints. We find that KM3-230213A gives stringent constraint on the DM mass ranging from GeV to GeV with lifetime in the range: s to s. Remarkably, in our SHDM scenario, the apparent tension between the KM3NeT observation and the nonobservation of this event by IceCube and Auger can be reduced to below . Our results are applicable to any neutrinophilic SHDM models while evading gamma-ray constraints.
v2: 5+3 pages, 3+1 captioned figures, 1 table, version accepted for publication as a Letter in Phys. Rev. D; v3: updated to match published version in Phys. Rev. D
References in corpus (21)
- Advanced LIGO
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array
- The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
- The NANOGrav 15-year Data Set: Search for Signals from New Physics
- IceCube-Gen2: The Window to the Extreme Universe
- The IceCube high-energy starting event sample: Description and flux characterization with 7.5 years of data
- Improved Characterization of the Astrophysical Muon-Neutrino Flux with 9.5 Years of IceCube Data
- Detection of a particle shower at the Glashow resonance with IceCube
- AugerPrime: the Pierre Auger Observatory Upgrade
- Search for Extremely-High-Energy Neutrinos and First Constraints on the Ultrahigh-Energy Cosmic-Ray Proton Fraction with IceCube
- Astronomy potential of KM3NeT/ARCA
- Heavy decaying dark matter at future neutrino radio telescopes
- Measurement of Very-high-energy Diffuse Gamma-ray Emissions from the Galactic Plane with LHAASO-WCDA
- Searches for Ultra-High-Energy Photons at the Pierre Auger Observatory
- Cascaded Gamma-ray Emission Associated with the KM3NeT Ultra-High-Energy Event KM3-230213A
- Neutrino lines from MeV dark matter annihilation and decay in JUNO
- Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
- Constraints on Lorentz-invariance violation in the neutrino sector from the ultrahigh-energy event KM3-230213A
- Thermal leptogenesis, dark matter, and gravitational waves from an extended canonical seesaw scenario
Cited by in corpus (11)
- Cosmological Origin of the KM3-230213A event and associated Gravitational Waves
- Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events
- Cosmic-Ray Constraints on the Flux of Ultra-High-Energy Neutrino Event KM3-230213A
- Superheavy Supersymmetric Dark Matter for the origin of KM3NeT Ultra-High Energy signal
- Ultra High Energy Neutrino Event KM3-230213A as a Signal of Electroweak Vacuum Turbulence in Merging Black Hole Binaries
- Cosmogenic Origin of KM3-230213A: Delayed Gamma-Ray Emission from A Cosmic-Ray Transient
- Exploring ultra-high energy neutrino experiments through the lens of the transport equation
- LHAASO Galactic Plane -rays Strongly Constrain Heavy Dark Matter
- Linking the KM3-230213A Neutrino Event to Dark Matter Decay and Gravitational Wave signals
- KM3-230213A and IceCube Neutrino Events from Metastable Dark Matter of Primordial Black Hole Origin
- Superluminal constraints from ultra-high-energy neutrino events