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

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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.
10 pages. 8 figures, 3 tables

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High Energy Physics - Phenomenology

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http://salesiana.dossiersoluciones.com/handle/123456789/204610

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0710.3125
 http://arxiv.org/abs/0710.3125
 Int.J.Mod.Phys.A23:2933-2942,2008
 doi:10.1142/S0217751X08041268

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arXiv