Abstract
Using sufficiently accurate uniform analytical approximations (applicable for all physically significant values of depths, zenith angles, and energies) of solutions to the equations of a simple model of a nuclear cascade in the atmosphere, formulas for the fluxes of mesons and muons for all depths (above sea level), energies, and zenith angles are derived.
Similar content being viewed by others
References
Gaisser, T.K., Cosmic Rays and Particle Physics, Cambridge: Univ. Press, 1990.
Chirkin, D., arXiv:hep-ph/0407078.
Popov, B.A. and Tesler, G.S., Vychislenie funktsii na EVM (Calculation of Functions with a PC), Kiev: Naukova Dumka, 1984.
Korn, G.A. and Korn, T.M., Mathematical Handbook for Scientists and Engineers, Dover Publ., 2000.
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © M.G. Kostyuk, 2017, published in Izvestiya Rossiiskoi Akademii Nauk, Seriya Fizicheskaya, 2017, Vol. 81, No. 7, pp. 1002–1004.
About this article
Cite this article
Kostyuk, M.G. Studying the muon flux with an analytically solvable model of a nuclear cascade in the atmosphere. Bull. Russ. Acad. Sci. Phys. 81, 907–909 (2017). https://doi.org/10.3103/S1062873817040281
Published:
Issue Date:
DOI: https://doi.org/10.3103/S1062873817040281