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LAN Xiao-gang, DING Lin-kai. Calibration for Energy Slope in Numerical Simulation of Cosmic Ray with High Energy[J]. Nuclear Physics Review, 2010, 27(1): 29-31. doi: 10.11804/NuclPhysRev.27.01.029
Citation: LAN Xiao-gang, DING Lin-kai. Calibration for Energy Slope in Numerical Simulation of Cosmic Ray with High Energy[J]. Nuclear Physics Review, 2010, 27(1): 29-31. doi: 10.11804/NuclPhysRev.27.01.029
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Calibration for Energy Slope in Numerical Simulation of Cosmic Ray with High Energy

doi: 10.11804/NuclPhysRev.27.01.029

  • 1 College of Physics and Electronic Information, China West Normal University, Nanchong 637002, Sichuan, China; 2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2010-03-20
  • In the study of hadronic interaction in the forward region by the simulation of cosmic ray, it is necessary to simulate large numbers of cosmic ray events with low first interaction height. We confirmed that by reducing the FIXCHI the efficiency of cosmic ray simulation can be improved. But the calibration for energy slope is needed. We got the energy slope based on the probability of direct arrived events with energy of 1 TeV, and fitted the intensity of spectrum with energy to make certain the energy slope of high energy cosmic ray. By this way, the efficiency and precision of cosmic ray simulation is greatly improved.
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Calibration for Energy Slope in Numerical Simulation of Cosmic Ray with High Energy

doi: 10.11804/NuclPhysRev.27.01.029
  • 1 College of Physics and Electronic Information, China West Normal University, Nanchong 637002, Sichuan, China; 2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2010-03-20

Abstract:  In the study of hadronic interaction in the forward region by the simulation of cosmic ray, it is necessary to simulate large numbers of cosmic ray events with low first interaction height. We confirmed that by reducing the FIXCHI the efficiency of cosmic ray simulation can be improved. But the calibration for energy slope is needed. We got the energy slope based on the probability of direct arrived events with energy of 1 TeV, and fitted the intensity of spectrum with energy to make certain the energy slope of high energy cosmic ray. By this way, the efficiency and precision of cosmic ray simulation is greatly improved.

LAN Xiao-gang, DING Lin-kai. Calibration for Energy Slope in Numerical Simulation of Cosmic Ray with High Energy[J]. Nuclear Physics Review, 2010, 27(1): 29-31. doi: 10.11804/NuclPhysRev.27.01.029
Citation: LAN Xiao-gang, DING Lin-kai. Calibration for Energy Slope in Numerical Simulation of Cosmic Ray with High Energy[J]. Nuclear Physics Review, 2010, 27(1): 29-31. doi: 10.11804/NuclPhysRev.27.01.029
shu

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