Milky Way as a Neutrino Desert Revealed by IceCube Galactic Plane Observation
Ke Fang, John S. Gallagher, Francis Halzen

TL;DR
This paper analyzes high-energy neutrino and gamma-ray data from the Galactic plane, revealing that the Milky Way's neutrino emission is significantly lower than that of distant galaxies, suggesting it is a neutrino desert.
Contribution
It demonstrates that the Milky Way's neutrino luminosity is much lower than extragalactic sources, indicating a lack of dominant neutrino emitters in our galaxy in recent times.
Findings
Neutrino flux from the Milky Way is 1-2 orders of magnitude lower than distant galaxies.
Gamma-ray observations are consistent with hadronuclear interactions above 1 TeV.
Our galaxy has not hosted dominant neutrino sources in the recent tens of kiloyears.
Abstract
The Galactic diffuse emission (GDE) is formed when cosmic rays leave the sources where they were accelerated, diffusively propagate in the Galactic magnetic field, and interact with the interstellar medium and interstellar radiation field. GDE in -ray (GDE-) has been observed up to sub-PeV energies, though its origin may be explained by either cosmic-ray nuclei or electrons. We show that the -rays accompanying the high-energy neutrinos recently observed by the IceCube Observatory from the Galactic plane have a flux that is consistent with the GDE- observed by the {\it Fermi}-LAT and Tibet AS experiments around 1 TeV and 0.5 PeV, respectively. The consistency suggests that the diffuse -ray emission above 1TeV could be dominated by hadronuclear interactions, though partial leptonic contribution cannot be excluded. Moreover, by…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Dark Matter and Cosmic Phenomena
