12-20 July 2017
BEXCO
Asia/Seoul timezone
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Contribution

BEXCO - Room F(201/202/203/204)

[CRI003] Simulation of horizontal tau-neutrino induced shower to optimize the site parameters

Speakers

  • Ali YILMAZ

Primary authors

  • Ali YILMAZ (Giresun University, Department of Electric and Electronics Engineering, 28200, Giresun, Turkey)

Co-authors

  • James RUSS (Carnegie-Mellon University, Pittsburgh, PA 15213, USA)
  • Umut KESKİN (Abant Izzet Baysal University, 14280 Bolu, Turkey)
  • Şeyma ATİK YILMAZ (Abant Izzet Baysal University, 14280 Bolu, Turkey)
  • Haluk DENİZLİ (Abant Izzet Baysal University, 14280 Bolu, Turkey)
  • Maurizio IORI (Sapienza University of Rome, Piazzale A. Moro 5, 00185 Rome, Italy, INFN, Sezione Roma 1, Piazzale A. Moro 2, 00185 Rome, It)
  • Kaan Yuksel OYULMAZ (Abant Izzet Baysal University, 14280 Bolu, Turkey)

Description

In the neutrino physics the direct measurement of the cosmogenic neutrino at energy of 10^15 − 1018 eV is still a challenging item. The most resent analysis of IceCube data results in an energy spectrum between 10^13 and 10^16 eV. We present the preliminary results of detailed Monte Carlo simulation of tau-induced air shower. In this study we consider the higher tau decay branching ratio (π−π0) at different energies (10^16 − 10^18 eV) generated by CORSIKA to evaluate the detection efficiency of the TAU-shoWER (TAUWER) array. It is designed as a future experiment for Ultra High Energetic tau-neutrino (UHE ντ ) astronomy to use Earth neutrino skimming strategy. The parameters (the distance from array plane to the emerging point and the neutrino energy) to optimize the detection efficiency and the trigger design for the TAUWER array setup are presented.