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arXiv:hep-ph/9803488·v3·High Energy Physics — Phenomenology

Atmospheric Muon Flux at Sea Level, Underground, and Underwater

E.V. Bugaev (1)🇷🇺 · A.Misaki (2)🇯🇵 · V.A.Naumov (3,4,5)🇷🇺 · T.S. Sinegovskaya (4)🇷🇺 · S.I. Sinegovsky (4)🇷🇺 · N.Takahashi (6) ((1) Institute for Nuclear Research, Moscow, (2) National Graduate Institute for Policy Studies, Urawa, (3) Lab of Theoretical Physics, Irkutsk State University, Irkutsk, (4) Physics Faculty, Irkutsk State University, Irkutsk, (5) INFN, Sezione di Firenze, Firenze, (6) Faculty of Science and Technology, Hirosaki University, Hirosaki)🇯🇵

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Abstract

The vertical sea-level muon spectrum at energies above 1 GeV and the underground/underwater muon intensities at depths up to 18 km w.e. are calculated. The results are particularly collated with a great body of the ground-level, underground, and underwater muon data. In the hadron-cascade calculations, the growth with energy of inelastic cross sections and pion, kaon, and nucleon generation in pion-nucleus collisions are taken into account. For evaluating the prompt muon contribution to the muon flux, we apply two phenomenological approaches to the charm production problem: the recombination quark-parton model and the quark-gluon string model. To solve the muon transport equation at large depths of homogeneous medium, a semi-analytical method is used. The simple fitting formulas describing our numerical results are given. Our analysis shows that, at depths up to 6-7 km w. e., essentially all underground data on the muon intensity correlate with each other and with predicted depth-intensity relation for conventional muons to within 10%. However, the high-energy sea-level data as well as the data at large depths are contradictory and cannot be quantitatively decribed by a single nuclear-cascade model.

Comments: 47 pages, REVTeX, 15 EPS figures included; recent experimental data and references added, typos corrected

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