Abstract
Sources of seasonal temperature variations in the average energy of the muon flux detected in the LVD experiment have been discussed. It has been shown that variations are due to the processes of generation of muons in upper layers of the atmosphere and the passage of muons through a thick rock layer.
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REFERENCES
M. Ambrosio et al. (MACRO Collab.), Astropart. Phys. 7, 109 (1997).
M. Selvi (for the LVD Collab.), in Proceedings of the 31st International Cosmic Ray Conference ICRC (2009), p. 1043.
C. Vigorito (for the LVD Collab.), in Proceedings of the 35th International Cosmic Ray Conference ICRC (2017), p. 291.
G. Bellini et al. (Borexino Collab.), J. Cosmol. Astropart. Phys. 1205, 015 (2012).
M. Agostini et al. (GERDA Collab.), Astropart. Phys. 84, 29 (2016).
P. Desiati (for the IceCube Collab.), in Proceedings of the 32nd International Cosmic Ray Conference ICRC (2011), p. 78.
P. Adamson et al. (MINOS Collab.), Phys. Rev. D 81, 012001 (2010).
T. Abrahão et al. (Double Chooz Collab.), J. Cosmol. Astropart. Phys. 1702, 017 (2017).
F.P. An et al., J. Cosmol. Astropart. Phys. 1801, 001 (2018).
N. Yu. Agafonova (on behalf of the LVD Collab.), arXiv:1701.04620; in Proceedings of the 25th European Cosmic Ray Symposium ECRS 2016, eConf C16-09-04.3.
A. S. Malgin, J. Exp. Theor. Phys. 121, 212 (2015).
N. Yu. Agafonova, Cand. Sci. (Phys. Math.) Dissertation (Inst. Nucl. Res. RAS, Moscow, 2015).
M. Ambrosio et al. (MACRO Collab.), Astropart. Phys. 19, 313 (2003).
M. Ambrosio et al. (MACRO Collab.), Phys. Rev. D 60, 032001 (1999).
J. Phys. G: Nucl. Part. Phys. 33, 1232 (2006).
D. E. Groom, N. V. Mokhov, and S. I. Striganov, At. Data Nucl. Data Tabl. 78, 183 (2001).
P. Lipari and T. Stanev, Phys. Rev. D 44, 3543 (1991).
O. M. Horn, PhD Thesis (Inst. Kernphys., Forschungszentrum Karlsruhe, Karlsruhe, 2008).
B. A. Kudryavtsev, Cand. Sci. (Phys. Math.) Dissertation (Inst. Nucl. Res. RAS, Moscow, 1998).
E. V. Bugaev, Yu. D. Kotov, and I. L. Rozental’, Cosmic Muons and Neutrinos (Atomizdat, Moscow, 1970) [in Russian].
V. V. Borog, V. G. Kirilov-Ugryumov, A. A. Petrukhin, et al., Sov. J. Nucl. Phys. 3, 575 (1966).
A. Malgin, Phys. Rev. C 96, 014605 (2017).
C. Castagnoli et al., Astropart. Phys. 6, 187 (1997).
M. Agostini et al., J. Cosmol. Astropart. Phys. 1902, 046 (2019).
E. V. Bugaev, A. Misaki, V. A. Naumov, T. S. Sinegovskaya, S. I. Sinegovsky, and N. Takahashi, Phys. Rev. D 58, 05401 (1998); arXiv: hep-ph/9803488v3.
C. Zhang and D.-M. Mei, Eur. Phys. J. C 79, 825 (2019).
Funding
This work was supported by the Russian Foundation for Basic Research (project no. 18-02-00064-a) and by the program of international cooperation between INFN (Italy) and the Ministry of Science and Higher Education of the Russian Federation.
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Translated by R. Tyapaev
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Agafonova, N.Y., Malgin, A.S. On the Mechanism of Temperature Variations in the Average Energy of Muons at Large Depths. J. Exp. Theor. Phys. 132, 73–78 (2021). https://doi.org/10.1134/S1063776121010088
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DOI: https://doi.org/10.1134/S1063776121010088