Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standard rock have been investigated using Geant4 simulation package. Muons with energies above 100 GeV were distributed from the ground level taking into account the muon charge ratio of similar to 1.3 at sea level. The simulated differential muon intensities are in good agreement with the intensities given in the literature. Furthermore, the simulation results for the integrated intensities are consistent with the experimental data, particularly at depths above 4000 m.w.e., where the simulation gives slightly smaller intensities than the experimental ones. In addition, the simulated exponent n at different underground depths agrees well with the ...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...
Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standa...
Recent measurements of the intensity of muons below 3000 m.w.e. (metres water equivalent) undergroun...
We have investigated the zenith angle distribution of muon intensities at three different depths of ...
With a pretty good-resolution mountain profile, we simulated the underground muon background at the ...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm-2...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm(-...
Geant4 simulation package was used to simulate muon fluxes at different locations, the floor of UNIR...
We have investigated the differential and integrated muon fluxes, muon charge ratios and the zenith ...
The production of neutrons by cosmic-ray muons at large depths underground is discussed. The most re...
Muon tomography is a method to investigate the in-situ rock density. It is based on the absorption o...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...
Underground muon intensities up to 10000 m.w.e. and angular distribution up to 6500 m.w.e. in standa...
Recent measurements of the intensity of muons below 3000 m.w.e. (metres water equivalent) undergroun...
We have investigated the zenith angle distribution of muon intensities at three different depths of ...
With a pretty good-resolution mountain profile, we simulated the underground muon background at the ...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm-2...
The vertical underground muon intensity has been measured in the slant depth range 3200-7000 hg cm(-...
Geant4 simulation package was used to simulate muon fluxes at different locations, the floor of UNIR...
We have investigated the differential and integrated muon fluxes, muon charge ratios and the zenith ...
The production of neutrons by cosmic-ray muons at large depths underground is discussed. The most re...
Muon tomography is a method to investigate the in-situ rock density. It is based on the absorption o...
The multiplicity spectrum of muon showers has been observed at depths of 1400-3400 hg/cm2 undergroun...
The angular and energy distributions of the primary cosmic rays that are responsible for the muons r...
Revtex4 33 pages, 16 figures and 4 tablesMuon backgrounds at Super-Kamiokande, KamLAND and CHOOZ are...