Pith. sign in

REVIEW 1 cited by

Galactic Diffuse Neutrino Emission from Sources beyond the Discovery Horizon

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

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

arxiv 2306.17285 v2 pith:LLPIHUIY submitted 2023-06-29 astro-ph.HE

Antonio Ambrosone , Kathrine M{o}rch Groth , Enrico Peretti , Markus Ahlers This is my paper · ORCID
classification astro-ph.HE
keywords emissionsourcesgalacticneutrinodiffuseicecubesignalunresolved
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The IceCube Neutrino Observatory has recently reported strong evidence for neutrino emission from the Galactic plane. The signal is consistent with model predictions of diffuse emission from cosmic ray propagation in the interstellar medium. However, due to IceCube's limited potential of identifying individual neutrino sources, it is also feasible that unresolved Galactic sources could contribute to the signal. We investigate the contribution of this quasi-diffuse emission and show that the observed Galactic diffuse flux at 100 TeV could be dominated by hard emission of unresolved sources. Particularly interesting candidate sources are young massive stellar clusters that have been considered as cosmic-ray PeVatrons. We examine whether this hypothesis can be tested by the upcoming KM3NeT detector or the planned future facility IceCube-Gen2 with about five times the sensitivity of IceCube.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Galactic Neutrino Sky: Predictions from Gamma-ray Source Populations

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    A template of resolved and unresolved gamma-ray sources, added to an unmodified diffuse model, reproduces the shape and spectrum of IceCube's inner-Galaxy neutrino excess.

Pith tools