arXiv · 0710.3125
High-energy Atmospheric Muon Flux Expected at India-Based Neutrino Observatory
Abstract
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.
Explore related subjects
Keep this discovery
Sukanta Panda, Sergei I. Sinegovsky. 2008-02-04. High-energy Atmospheric Muon Flux Expected at India-Based Neutrino Observatory. https://doi.org/10.1142/s0217751x08041268
Cite the original work for its findings. Save a collection to share your selection of sources.