Systematic differences due to high energy hadronic interaction models in air shower simulations in the 100 GeV-100 TeV range

نویسندگان
چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Comparison of high energy interaction models used for atmospheric shower simulations above 1 TeV

We present here a comparison of interaction models commonly used for simulating cosmic ray shower development in the atmosphere at energies greater than 1 TeV. The implementations of these models in CORSIKA and the FLUKA transport and interaction code are relevant for extensive air shower experiments, neutrino telescopes, and gamma-ray surfacebased detectors. We compare the pion, kaon, charmed ...

متن کامل

Influence of Low Energy Hadronic Interactions on Air-shower Simulations

Experiments measuring cosmic rays above an energy of ∼ 10 eV deduce the energy and mass of the primary cosmic ray particles from air-shower simulations. We investigate the importance of hadronic interactions at low and high energies on the distributions of muons and electrons in showers on ground. In air shower simulation programs, hadronic interactions below an energy threshold in the range fr...

متن کامل

Hadronic interaction models and the air shower simulation program CORSIKA

The Monte Carlo program CORSIKA simulates the 4-dimensional evolution of extensive air showers in the atmosphere initiated by photons, hadrons or nuclei. It contains links to the hadronic interaction models DPMJET, HDPM, NEXUS, QGSJET, SIBYLL, and VENUS. These codes are employed to treat the hadronic interactions at energies above 80 GeV. Since their first implementation in 1996 the models DPMJ...

متن کامل

Tests of hadronic interaction models by data of the KASCADE-Grande air-shower experiment

A. Haungs, M. Risse, W.D. Apel, F. Badea, K. Bekk, J. Blümer, H. Bozdog, K. Daumiller, P. Doll, R. Engel, J. Engler, H.J. Gils, D. Heck, J.R. Hörandel, T. Huege, H.O. Klages, G. Maier, H.J. Mathes, H.J. Mayer, J. Milke, M. Müller, S. Nehls, R. Obenland, J. Oehlschläger, S. Ostapchenko, T. Pierog, S. Plewnia, H. Rebel, M. Roth, H. Schieler, M. Stümpert, H. Ulrich, J. van Buren, A. Weindl, J. Woc...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Physical Review D

سال: 2019

ISSN: 2470-0010,2470-0029

DOI: 10.1103/physrevd.100.023010