MONTE-CARLO SIMULATION OF COSMIC RAY ANTIPROTON INTENSITY
- Received Date: 1979-10-07
- Accepted Date: 1900-01-01
- Available Online: 1980-12-05
Abstract: Using Monte-Carlo method, the propagation of cosmic ray hadrons throughatmosphere is simulated. The aim is to study. the production of NN in strong interac-tions beyond the accelerator energy range and to see whether there is certain fractionof antiprotons by means of comparing the calculated and measured cosmic ray anti-proton intensity at 3200m above sea level. The calculated spectra of cosmic ray p,π±,μ at mountain altitude and at sea level are shown to agree with the measured ones.Some discussions on the results are given.