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Improved Characterization of the Astrophysical Muon-neutrino Flux with 9.5 Years of IceCube Data
Journal article   Open access

Improved Characterization of the Astrophysical Muon-neutrino Flux with 9.5 Years of IceCube Data

Maryon Ahrens, Kunal Deoskar, Chad Finley, Klas Hultqvist, Matti Jansson, Christian Walck and IceCube Collaboration
The Astrophysical journal, v 928(1)
2022
url
https://doi.org/10.3847/1538-4357/ac4d29View
Published, Version of Record (VoR) Open CC BY V4.0

Abstract

Fysik Naturvetenskap Subatomic Physics Subatomär fysik ESI Highly Cited Paper (Incites) Natural Sciences Physical Sciences
We present a measurement of the high-energy astrophysical muon-neutrino flux with the IceCube Neutrino Observatory. The measurement uses a high-purity selection of 650k neutrino-induced muon tracks from the northern celestial hemisphere, corresponding to 9.5 yr of experimental data. With respect to previous publications, the measurement is improved by the increased size of the event sample and the extended model testing beyond simple power-law hypotheses. An updated treatment of systematic uncertainties and atmospheric background fluxes has been implemented based on recent models. The best-fit single power-law parameterization for the astrophysical energy spectrum results in a normalization of phi(nu mu+(nu) over bar mu)(@ 00TeV) = 1.441(-0.26)(+0.25 )x 10(-18) GeV(-1)cm(-2) s(-1 )sr(-1) and a spectral index gamma(SPL) = 2.37(-0.09)(+0.09), constrained in the energy range from 15 TeV to 5 PeV. The model tests include a single power law with a spectral cutoff at high energies, a log-parabola model, several source-class-specific flux predictions from the literature, and a model-independent spectral unfolding. The data are consistent with a single power-law hypothesis, however, spectra with softening above one PeV are statistically more favorable at a two-sigma level.

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Collaboration types
Domestic collaboration
International collaboration
Web of Science research areas
Astronomy & Astrophysics
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