Zhurnal Tekhnicheskoi Fiziki, 2023 Volume 93, Issue 12, Pages 1807–1810
(Mi jtf7177)
International Conference PhysicA.SPb 23-27 October, 2023 St. Petersburg
Astronomy and Astrophysics
Simulation of Tunka-Grande and TAIGA-Muon scintillation facilities
M. Yu. Ternovoy a ,
I. I. Astapov b ,
P. A. Bezyazeekov a ,
E. A. Bonvech c ,
A. N. Borodin d ,
N. M. Budnev a ,
A. V. Bulan c ,
N. V. Volkov e ,
P. A. Volchugov c ,
D. M. Voronin f ,
A. R. Gafarov a ,
E. O. Gress a ,
O. A. Gress a ,
T. I. Gress a ,
O. G. Grishin a ,
A. Yu. Garmash g ,
V. M. Grebenyuk dh ,
A. A. Grinyuk d ,
A. N. Dyachok a ,
D. P. Zhurov ai ,
A. V. Zagorodnikov a ,
A. D. Ivanova aj ,
A. L. Ivanova ag ,
M. A. Ilyushin a ,
N. N. Kalmykov c ,
V. V. Kindin a ,
S. N. Kiryukhin a ,
R. P. Kokoulin b ,
N. I. Kolosov a ,
K. G. Kompaniets b ,
E. E. Korosteleva c ,
V. A. Kozhin c ,
E. A. Kravchenko gk ,
A. P. Kryukov c ,
L. A. Kuzmichev c ,
A. A. Lagutin e ,
M. V. Lavrova d ,
Yu. E. Lemeshev a ,
B. K. Lubsandorzhiev f ,
N. B. Lubsandorzhiev c ,
S. D. Malakhov a ,
R. R. Mirgazov a ,
R. D. Monkhoev a ,
E. A. Okuneva c ,
E. A. Osipova c ,
A. L. Pakhorukov a ,
A. Pan d ,
A. D. Panov c ,
L. V. Pan'kov a ,
A. A. Petrukhin b ,
D. A. Podgrudkov c ,
E. G. Popova c ,
E. B. Postnikov c ,
V. V. Prosin c ,
V. S. Ptuskin l ,
A. A. Pushnin a ,
A. V. Razumov c ,
R. I. Raikin e ,
G. I. Rubtsov f ,
E. V. Rjabov a ,
V. S. Samoliga a ,
I. Satyshev d ,
A. A. Silaev c ,
A. A. Silaev (junior) c ,
A. Yu. Sidorenkov f ,
A. V. Skurihin c ,
A. V. Sokolov gk ,
L. G. Sveshnikova c ,
V. A. Tabolenko a ,
A. B. Tanaev a ,
L. G. Tkachev dh ,
N. A. Ushakov f ,
D. V. Chernov c ,
I. I. Yashin b ,
A. Chiavassa m ,
A. Vaydyanatan g a Institute of Applied Physics, Irkutsk State University,
664000 Irkutsk, Russia
b National Engineering Physics Institute "MEPhI", 115409 Moscow, Russia
c Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics, 119991 Moscow, Russia
d Joint Institute for Nuclear Research, Dubna, Moscow region, 141980 Dubna, Russia
e Altai State University, 656049 Barnaul, Russia
f Institute for Nuclear Research, Russian Academy of Sciences, 117312 Moscow, Russia
g Novosibirsk State University, 630090 Novosibirsk, Russia
h Dubna State University, 141982 Dubna, Russia
i Irkutsk State Technical University, 664074 Irkutsk, Russia
j Moscow Institute of Physics and Technology (National Research University), 141701 Moscow, Russia
k G I. Budker Institute of Nuclear Physics, Siberian Branch of the Russian Academy of Sciences, 630090 Novosibirsk, Russia
l Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, 108840 Moscow, Russia
m University of Turin
Abstract:
A planning for computer generated simulation of scintillation equipment based on the CORSIKA and Geant4 software packages is presented. Method developed to optimize the simulation process is presented. A possible approach for determining the mass composition of charged cosmic rays is discussed. Preliminary results of computer generated of the Tunka-Grande installation in the energy range 10–100 PeV are also presented.
Keywords:
experimental complex TAIGA, cosmic rays, wide atmospheric showers, mass composition, CORSIKA, Geant4. Received: 12.05.2023
Revised: 03.09.2023
Accepted: 30.10.2023
DOI:
10.61011/JTF.2023.12.56827.f237-23
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