Examination of Calculations of the Atmospheric Muon and Neutrino Spectra Using New Measurements
- 作者: Kochanov A.A.1,2, Morozova A.D.3,4, Sinegovskaya T.S.5, Sinegovsky S.I.2,3
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隶属关系:
- Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences
- Irkutsk State University
- Joint Institute for Nuclear Research
- Moscow State University
- Irkutsk State Transport University
- 期: 卷 83, 编号 8 (2019)
- 页面: 933-936
- 栏目: Article
- URL: https://journals.rcsi.science/1062-8738/article/view/187480
- DOI: https://doi.org/10.3103/S1062873819080203
- ID: 187480
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详细
The atmospheric muon and neutrino fluxes at energies from 10 GeV to 10 PeV are calculated with the Kimel–Mokhov (KM), SIBYLL 2.1, EPOS LHC, and QGSJET-II hadronic models for known parameterizations of the cosmic ray spectra by Zatsepin--Sokolskaya and Hillas–Gaisser. The calculations with the KM, EPOS LHC, and SIBYLL 2.1 models are agree well with the measurements of the atmospheric muon spectra in IceCube and IceTop experiments. The measurement of high-energy muon spectra indicates the presence of the prompt muon component at energies above 500 TeV, which is well reproduced in calculations with the quark-gluon string model. The calculations of the atmospheric muon neutrino spectrum performed for the KM, EPOS LHC, and SIBYLL 2.1 models give good fit with the measurement data of IceCube, ANTARES, and Super-Kamiokande experiments.
作者简介
A. Kochanov
Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences; Irkutsk State University
编辑信件的主要联系方式.
Email: kochanov@iszf.irk.ru
俄罗斯联邦, Irkutsk, 664033; Irkutsk, 664003
A. Morozova
Joint Institute for Nuclear Research; Moscow State University
Email: kochanov@iszf.irk.ru
俄罗斯联邦, Dubna, 141980; Moscow, 119991
T. Sinegovskaya
Irkutsk State Transport University
Email: kochanov@iszf.irk.ru
俄罗斯联邦, Irkutsk, 664074
S. Sinegovsky
Irkutsk State University; Joint Institute for Nuclear Research
Email: kochanov@iszf.irk.ru
俄罗斯联邦, Irkutsk, 664003; Dubna, 141980
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