Status of the Scintillation Experiment of the TAIGA Astrophysical Complex

IF 0.4 4区 物理与天体物理 Q4 PHYSICS, NUCLEAR
E. A. Kravchenko, I. I. Astapov, P. A. Bezyazeekov, E. A. Bonvech, A. Blinov, A. N. Borodin, N. M. Budnev, A. V. Bulan, P. V. Busygin, D. V. Chernov, A. Chiavassa, A. N. Dyachok, V. A. Erofeeva, A. R. Gafarov, A. Yu. Garmash, V. M. Grebenyuk, E. O. Gress, O. A. Gress, T. I. Gress, A. A. Grinyuk, O. G. Grishin, A. D. Ivanova, A. L. Ivanova, M. A. Iliushin, I. A. Kabannik, N. N. Kalmykov, V. V. Kindin, S. N. Kiryukhin, N. I. Kolosov, K. G. Kompaniets, E. E. Korosteleva, V. A. Kozhin, A. P. Kryukov, L. A. Kuzmichev, A. A. Lagutin, M. V. Lavrova, Yu. E. Lemeshev, B. K. Lubsandorzhiev, N. Lubsandorzhiev, A. Lukanov, S. D. Malakhov, R. R. Mirgazov, R. D. Monkhoev, E. A. Okuneva, E. A. Osipova, A. L. Pakhorukov, L. V. Pankov, A. Pan, A. D. Panov, A. A. Petrukhin, D. A. Podgrudkov, I. Poddubny, V. A. Poleschuk, E. G. Popova, E. B. Postnikov, V. V. Prosin, A. A. Pushnin, R. I. Raikin, A. V. Razumov, G. I. Rubtsov, E. V. Ryabov, V. S. Samoliga, I. Satyshev, A. A. Silaev,  A. A. Silaev, A. Yu. Sidorenkov, A. V. Skurikhin, A. V. Sokolov, L. G. Sveshnikova, A. Shaikovsky, M. V. Shulga, V. A. Tabolenko, L. G. Tkachev, A. B. Tanaev, M. Yu. Ternovoy, N. A. Ushakov, P. A. Volchugov, N. V. Volkov, D. M. Voronin, V. Zirakashvili, A. V. Zagorodnikov, D. P. Zhurov, I. I. Yashin
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引用次数: 0

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.

Abstract Image

TAIGA天体物理复合体闪烁实验现状
TAIGA天体物理复合体的闪烁实验包括两个系统:Tunka-Grande和TAIGA - muon。这些系统的主要目标是研究\(10^{15}{-}10^{18}\) eV能量范围内宇宙射线的能谱和质量组成,以及在同一能量范围内寻找伽马辐射。实验的另一项任务是与广角切伦科夫探测器TAIGA-HiSCORE和Tunka-133一起寻找亚pev能量范围内的伽马量子信号。该报告介绍了该设施的目标和现状,并描述了闪烁计数器和簇的设计。本文介绍了具有不同寻常时空结构的EAS的研究结果,以及Tunka-Grande和TAIGA-HiSCORE装置联合操作以搜索亚pev伽马量子的研究结果。估计是由蟹状星云中预期的注册伽马量子数做出的。
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来源期刊
Physics of Atomic Nuclei
Physics of Atomic Nuclei 物理-物理:核物理
CiteScore
0.60
自引率
25.00%
发文量
56
审稿时长
3-6 weeks
期刊介绍: Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.
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