All-particle energy spectrum of KASCADE-Grande based on shower size and different hadronic interaction models

نویسندگان

  • D Kang
  • W D Apel
  • J C Arteaga-Velázquez
  • K Bekk
  • M Bertaina
  • J Blümer
  • H Bozdog
  • I M Brancus
  • E Cantoni
  • A Chiavassa
  • F Cossavella
  • K Daumiller
  • V de Souza
  • F Di Pierro
  • P Doll
  • R Engel
  • J Engler
  • M Finger
  • B Fuchs
  • D Fuhrmann
  • H J Gils
چکیده

KASCADE-Grande is a large detector array for observations of the energy spectrum as well as the chemical composition of cosmic ray air showers up to primary energies of 1 EeV. The multi-detector arrangement allows to measure the electromagnetic and muonic components for individual air showers. In this analysis, the reconstruction of the all-particle energy spectrum is based on the size spectra of the charged particle component. The energy is calibrated by using Monte Carlo simulations performed with CORSIKA and high-energy interaction models QGSJet, EPOS and SIBYLL. In all cases FLUKA has been used as lowenergy interaction model. In this contribution the resulting spectra by means of different hadronic interaction models will be compared and discussed. 23rd European Cosmic Ray Symposium (and 32nd Russian Cosmic Ray Conference) IOP Publishing Journal of Physics: Conference Series 409 (2013) 012101 doi:10.1088/1742-6596/409/1/012101 Published under licence by IOP Publishing Ltd 1

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تاریخ انتشار 2017