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The Astrophysical Journal
Article . 2023 . Peer-reviewed
License: CC BY
Data sources: Crossref
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https://dx.doi.org/10.5445/ir/...
Article . 2023
License: CC BY
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Search for Extended Sources of Neutrino Emission in the Galactic Plane with IceCube

Authors: IceCube Collaboration; Abbasi, R.; Ackermann, M.; Adams, J.; Agarwalla, S. K.; Aguilar, J. A.; Ahlers, M.; +193 Authors

Search for Extended Sources of Neutrino Emission in the Galactic Plane with IceCube

Abstract

Abstract The Galactic plane, harboring a diffuse neutrino flux, is a particularly interesting target in which to study potential cosmic-ray acceleration sites. Recent gamma-ray observations by HAWC and LHAASO have presented evidence for multiple Galactic sources that exhibit a spatially extended morphology and have energy spectra continuing beyond 100 TeV. A fraction of such emission could be produced by interactions of accelerated hadronic cosmic rays, resulting in an excess of high-energy neutrinos clustered near these regions. Using 10 years of IceCube data comprising track-like events that originate from charged-current muon neutrino interactions, we perform a dedicated search for extended neutrino sources in the Galaxy. We find no evidence for time-integrated neutrino emission from the potential extended sources studied in the Galactic plane. The most significant location, at 2.6σ post-trials, is a 1.°7 sized region coincident with the unidentified TeV gamma-ray source 3HWC J1951+266. We provide strong constraints on hadronic emission from several regions in the galaxy.

Countries
Belgium, Belgium, Sweden, Italy, Germany, Denmark
Keywords

astro-ph.GA, energy spectrum, FOS: Physical sciences, Astrophysics, 530, neutrino: flux, High Energy Physics - Experiment, IceCube, charged current, Subatomär fysik, High Energy Physics - Experiment (hep-ex), Astronomi, astrofysik och kosmologi, muon, Subatomic Physics, site, Astronomy, Astrophysics and Cosmology, TeV, cosmic radiation: acceleration, info:eu-repo/classification/ddc/530, LHAASO, neutrino: interaction, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), hep-ex, Physics, ddc:530, neutrino: particle source, Astrophysics - Astrophysics of Galaxies, 520, QB460-466, Physics and Astronomy, Neutrino astronomy, gamma ray, Astrophysics of Galaxies (astro-ph.GA), galaxy, Astrophysics - High Energy Astrophysical Phenomena, info:eu-repo/classification/ddc/520, HAWC

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
7
Top 10%
Average
Top 10%