High-energy Atmospheric Muon Flux Expected at India-Based Neutrino Observatory

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dc.creatorPanda, Sukanta
dc.creatorSinegovsky, Sergei I.
dc.date2007-10-16
dc.date2008-02-04
dc.date.accessioned2026-07-07T11:53:38Z
dc.date.available2026-07-07T11:53:38Z
dc.descriptionWe 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.
dc.description10 pages. 8 figures, 3 tables
dc.identifierhttps://arxiv.org/abs/0710.3125
dc.identifierhttp://arxiv.org/abs/0710.3125
dc.identifierInt.J.Mod.Phys.A23:2933-2942,2008
dc.identifierdoi:10.1142/S0217751X08041268
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204610
dc.subjectHigh Energy Physics - Phenomenology
dc.titleHigh-energy Atmospheric Muon Flux Expected at India-Based Neutrino Observatory
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