Prospects for detecting galactic sources of cosmic neutrinos with IceCube: An update

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• 作者：Francis Halzen^a ; ^{francis.halzen@icecube.wisc.edu} ; Ali Kheirandish^a ; ^{ali.kheirandish@icecube.wisc.edu} ; Viviana Niro ; ^b ; ^{viviana.niro@uam.es}
• 关键词：High-energy neutrinos ; Neutrino astronomy ; High-energy cosmic-ray physics and astrophysics
• 刊名：Astroparticle Physics
• 出版年：2017
• 出版时间：January 2017
• 年：2017
• 卷：86
• 期：Complete
• 页码：46-56
• 全文大小：963 K
• 卷排序：86

文摘

Air-Cherenkov telescopes have mapped the Galactic plane at TeV energies. Here we evaluate the prospects for detecting the neutrino emission from sources in the Galactic plane assuming that the highest energy photons originate from the decay of pions, which yields a straightforward prediction for the neutrino flux from the decay of the associated production of charged pions. Four promising sources are identified based on having a large flux and a flat spectrum. We subsequently evaluate the probability of their identification above the atmospheric neutrino background in IceCube data as a function of time. We show that observing them over the twenty-year lifetime of the instrumentation is likely, and that some should be observable at the 3 σ level with six years of data. In the absence of positive results, we derive constraints on the spectral index and cut-off energy of the sources, assuming a hadronic acceleration mechanism.