Theoretical calculations estimate cascade spectra from atmospheric muons in a neutrino telescope, supporting background assessment for ultra-high-energy neutrino detection.
This paper presents the results of computer simulations and theoretical calculations of cascade showers generated by atmospheric muons in the Baikal-GVD neutrino telescope. Cascade spectra are required to estimate the background in the search for ultra-high-energy neutrinos and can be used to measure the atmospheric muon spectrum in the ultra-high-energy region.
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Lisitsin et al. (2026) studied this question.
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