Journal
ASTROPARTICLE PHYSICS
Volume 25, Issue 1, Pages 1-13Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.astropartphys.2005.10.005
Keywords
atmospheric muon flux; underwater muon energy spectrum; multiple muons; neutrino telescopes
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Atmospheric muons play an important role in underwater/ice neutrino detectors. In this paper, a parameterisation of the flux of single and multiple muon events, their lateral distribution and of their energy spectrum is presented. The kinematics parameters were modelled starting from a full Monte Carlo simulation of the interaction of primary cosmic rays with atmospheric nuclei; secondary muons reaching the sea level were propagated in the deep water. The parametric formulas are valid for a vertical depth of 1.5-5 km.w.e. and lip to 85 degrees for the zenith angle, and can be used as input for a fast simulation of atmospheric muons in underwater/ice detectors. (c) 2005 Elsevier B.V. All rights reserved.
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