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High-energy Atmospheric Muon Flux Expected at India-Based Neutrino Observatory
We calculate the zenith-angle dependence of conventional and prompt
high-energy muon fluxes at India-Based Neutrino Observatory (INO) depth. This
study demonstrates a possibility to discriminate models of the charm
hadroproduction including the low-x QCD behaviour of hadronic cross-sections
relevant at very high energies.Comment: 10 pages. 8 figures, 3 table
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