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 up to 85^ for the zenith angle, and can be used as input for a fast simulation of atmospheric muons in underwater/ice detectors.
Y. Becherini, A. Margiotta, M. Sioli, M. Spurio (2006). A parameterisation of single and multiple muons in the deep water or ice. ASTROPARTICLE PHYSICS, 25, 1-13 [10.1016/j.astropartphys.2005.10.005].
A parameterisation of single and multiple muons in the deep water or ice
BECHERINI, YVONNE;MARGIOTTA, ANNARITA;SIOLI, MAXIMILIANO;SPURIO, MAURIZIO
2006
Abstract
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 up to 85^ for the zenith angle, and can be used as input for a fast simulation of atmospheric muons in underwater/ice detectors.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
