Status of the Scintillation Experiment of the TAIGA Astrophysical Complex

The scintillation experiment of the TAIGA astrophysical complex comprises two systems: Tunka-Grande and Taiga-Muon. The main objective of these systems is to study the energy spectrum and mass composition of cosmic rays in the energy range of $$10^{15}{-}10^{18}$$ eV, as well as to search for gamma radiation in the same energy range. An additional task of the experiments is to search for a signal from gamma quanta in the sub-PeV energy range in conjunction with wide angle Cherenkov detectors TAIGA-HiSCORE and Tunka-133. The report presents the objectives and status of the facility and a description of the design of scintillation counters and clusters. The results of the study of EAS with an unusual spatiotemporal structure are presented together with the results of a study of the joint operation of the Tunka-Grande and TAIGA-HiSCORE setups in order to search for sub-PeV gamma quanta. Estimates are made of the expected number of registered gamma quanta from the Crab Nebula.

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Journal
Physics of Atomic Nuclei
Published
2025-04-01
DOI
https://doi.org/10.1134/s1063778825600496
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

Status of the Scintillation Experiment of the TAIGA Astrophysical Complex

A. P. Kryukov, И. И. Астапов, Д. Журов, В. А. Кожин et al.
Physics of Atomic Nuclei
Astrophysics and Cosmic Phenomena
article

Status of the Scintillation Experiment of the TAIGA Astrophysical Complex

A. P. Kryukov, И. И. Астапов, Д. Журов, В. А. Кожин, К. Г. Компаниец, P. A. Bezyazeekov, Andrey Sidorenkov, А. А. Петрухин, N. Lubsandorzhiev, А. Пушнин, I. I. Yashin, L. Pankov, В. Самолига, Л. Г. Свешникова, M. Ternovoy, I. Poddubny, Nikita Ushakov, V. Prosin, Yu. Lemeshev, Е. А. Бонвеч, А. Р. Гафаров, А. Пан, В. В. Киндин, S. N. Kiryukhin, Н. Н. Калмыков, A. D. Ivanova, А. В. Скурихин, Р. Р. Миргазов, V. Poleschuk, L. A. Kuzmichev, А. Д. Панов, А. Танаев, A. V. Zagorodnikov, Н. И. Колосов, A. N. Dyachok, Т. И. Гресс, Е. Постников, А. Пахоруков, V. Grebenyuk, Д. Воронин, A. A. Grinyuk, M. V. Lavrova, Victoria Erofeeva, Г. И. Рубцов, Р. И. Райкин, A. L. Ivanova, Л. Ткачев, А. Булан, О. Гришин, А. Бородин, А. В. Блинов, A. Lukanov, И. Сатышев, Д. В. Чернов, E. Gress, V. N. Zirakashvili, E. V. Ryabov, N. M. Budnev, А. А. Силаев, П. А. Волчугов, Е. Е. Коростелева, Н. В. Волков, A. Sokolov, О. Гресс, М. А. Илюшин, P. V. Busygin, A. Chiavassa, Е. Г. Попова, Е. А. Кравченко, В. А. Таболенко, Р. Д. Монхоев, A. Garmash, Б. К. Лубсандоржиев, А. А. Лагутин, Э. А. Окунева, С. Д. Малахов, Д. Подгрудков, Э. А. Осипова, М.В. Шульга, A. V. Razumov, A. Shaikovsky, I. A. Kabannik
article en

Abstract

The scintillation experiment of the TAIGA astrophysical complex comprises two systems: Tunka-Grande and Taiga-Muon. The main objective of these systems is to study the energy spectrum and mass composition of cosmic rays in the energy range of $$10^{15}{-}10^{18}$$ eV, as well as to search for gamma radiation in the same energy range. An additional task of the experiments is to search for a signal from gamma quanta in the sub-PeV energy range in conjunction with wide angle Cherenkov detectors TAIGA-HiSCORE and Tunka-133. The report presents the objectives and status of the facility and a description of the design of scintillation counters and clusters. The results of the study of EAS with an unusual spatiotemporal structure are presented together with the results of a study of the joint operation of the Tunka-Grande and TAIGA-HiSCORE setups in order to search for sub-PeV gamma quanta. Estimates are made of the expected number of registered gamma quanta from the Crab Nebula.

Physics of Atomic NucleiVol. 88(2)
Moscow Institute of Physics and Technology (RU), Altai State University (RU), Novosibirsk State University (RU), Joint Institute for Nuclear Research (RU), Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation (RU), Dubna State University (RU), Institute for Nuclear Research (RU), Siberian Branch of the Russian Academy of Sciences (RU), Budker Institute of Nuclear Physics (RU), University of Turin (IT), National Research Nuclear University MEPhI (RU), Irkutsk State University (RU)
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