Energy Spectrum of Primary Cosmic Rays According to the Data of the TAIGA Astrophysical Complex

V. V. Prosin, I. I. Astapov, P. A. Bezyazeekov, E. A. Bonvech,A. N. Borodin,N. M. Budnev, A. V. Bulan, D. V. Chernov, A. Chiavassa, A. N. Dyachok, A. R. Gafarov,A. Yu. Garmash, V. M. Grebenyuk,E. O. Gress,O. A. Gress, T. I. Gress, A. A. Grinyuk, O. G. Grishin, M. A. Iliushin,A. D. Ivanova,A. L. Ivanova,N. N. Kalmykov,V. V. Kindin, S. N. Kiryuhin, R. P. Kokoulin, N. I. Kolosov, K. G. Kompaniets, E. E. Korosteleva, V. A. Kozhin,E. A. Kravchenko, A. P. Kryukov,L. A. Kuzmichev, A. A. Lagutin, M. V. Lavrova,Yu. E. Lemeshev, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, S. D. Malakhov,R. R. Mirgazov, R. A. Monkhoev, E. A. Okuneva, E. A. Osipova, A. L. Pakhorukov,A. Pan, A. D. Panov, L. V. Pankov,A. A. Petrukhin, D. A. Podgrudkov, E. G. Popova, E. B. Postnikov, V. S. Ptuskin, A. A. Pushnin,R. I. Raikin, A. V. Razumov, E. V. Rjabov, G. I. Rubtsov, V. S. Samoliga, I. Satyshev,A. Yu. Sidorenkov,A. A. Silaev,A. A. Silaev Jr., A. V. Skurikhin,A. V. Sokolov,L. G. Sveshnikova, V. A. Tabolenko,A. B. Tanaev, B. A. Tarashansky, M. Yu. Ternovoy, L. G. Tkachev,N. A. Ushakov, A. Vaidyanathan,N. V. Volkov, P. A. Volchugov, D. M. Voronin, I. I. Yashin, A. V. Zagorodnikov,D. P. Zhurov

Bulletin of the Russian Academy of Sciences: Physics（2023）

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摘要

The more correct recalculation from the measured Cherenkov light fluxes at distances of 200 (Q200) and 100 (Q100) m from the Extensive Air Shower (EAS) core to the energy of the primary particle has been developed using the results of M-C simulation by the CORSIKA code, assuming a light primary composition of cosmic rays. Using the new conversion expressions, a differential energy spectrum was obtained according to the data of the Tunka-133 array for 7 years of operation and the TAIGA-HiSCORE array for 2 years of operation.

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关键词

extensive air shower,Cerenkov light flux,primary particle energy spectrum

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