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SUMMARY:Testing of the DPMJET and VENUS hadronic interaction models with t
 he help of the atmospheric muons
DTSTART;VALUE=DATE-TIME:20161012T143000Z
DTEND;VALUE=DATE-TIME:20161012T144500Z
DTSTAMP;VALUE=DATE-TIME:20260713T101632Z
UID:indico-contribution-534@cern.ch
DESCRIPTION:Speakers: Anton Lukyashin (ITEP\, NRNU MEPhI)\nThe more accura
 te original calculations of the atmospheric vertical energy spectrum at en
 ergies $10^{2} - 10^{5} \\space $ GeV have been carried out in terms of DP
 MJET $~2.55 \\space $ and VENUS $~4.12 \\space $ models. The Gaisser-Honda
  approximation and results of measurements of energy of primary protons\, 
 helium and nitrogen nuclei has been used. The package  CORSIKA $~7.4 \\spa
 ce $  has been used to simulate in the standard atmosphere cascades induce
 d by different primary particles with various fixed energies $E_{0} \\spac
 e $. Statistics of simulated cascades for secondary particles with energie
 s (0.01–1)$ \\cdot E_{0} \\space $ was increased up to $10^{6} \\space $
 . The results of simulations have been compared with data. This fit showed
  how the used models have been changed.\n\nhttps://indico.particle.mephi.r
 u/event/4/contributions/534/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/534/
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