REVIEW 6 cited by
What KM3-230213A events may tell us about the neutrino mass and dark matter
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
abstract
Within the framework of general $U(1)$ scenario, we demonstrate that the ultra high energy neutrinos recently detected by KM3NeT could originate from a decaying right handed neutrino dark matter (DM), with a mass of 440 PeV. Considering DM production via freeze-in, we delineate the parameter space that satisfies the observed relic abundance and also lies within the reach of multiple gravitational wave detectors. Our study provides a testable new physics scenario, enabled by multi-messenger astronomy.
Forward citations
Cited by 6 Pith papers
-
Earth rotation turns event timing into a geometric probe of UHE neutrino origin
Earth-rotation timing lowers the number of future KM3NeT events needed to exclude a dark-matter origin of KM3-230213A from ~22–27 to ~14–16.
-
Constraining Gravitational Dark Matter with LHAASO and Fermi-LAT
Diffuse Galactic gamma-ray data strongly limit the couplings of gravitationally produced decaying dark matter, and the paper claims an oscillation-based bound on massive dark photons.
-
`Dark' Matter Effect as a Novel Solution to the KM3-230213A Puzzle
Dark matter scattering in the Earth, sourced by a flaring blazar, can explain the KM3-230213A event while yielding few or no IceCube events in a viable parameter space.
-
Astrophysical flux of dark particles as a solution to the KM3NeT and IceCube tension over KM3-230213A
A transient astrophysical dark-particle flux can explain the KM3NeT 70 PeV muon via in-Earth upscattering and decay to muon pairs, while predicting no IceCube counterpart.
-
Breaking Dark: Hunting Heavy Decaying Dark Matter with Tibet AS$_\gamma$ and LHAASO-KM2A
Tibet ASγ and LHAASO-KM2A diffuse gamma-ray data exclude decaying dark matter lifetimes below about 10^28 seconds for masses around 10^6-10^9 GeV, for many Standard Model final states.
-
Exploring ultra-high energy neutrino experiments through the lens of the transport equation
Using a line-of-sight transport formalism, the paper finds a 3.1 sigma tension between the KM3NeT ultra-high-energy event and IceCube non-observation under a diffuse power-law flux, with stronger tension for steady po...
Discussion (0). Continue with ORCID to comment.