High-Energy Cosmic-Ray Muons Under Thick Layers of Matter I. a Method to Solve the Transport Equation

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dc.creatorNaumov, V. A.
dc.creatorSinegovsky, S. I.
dc.creatorBugaev, E. V.
dc.date1993-01-22
dc.date.accessioned2026-07-07T03:55:56Z
dc.date.available2026-07-07T03:55:56Z
dc.descriptionAn effective analytical method for calculating energy spectra of cosmic-ray muons at large depths of homogeneous media is developed. The method allows to include an arbitrary (decreasing) muon spectrum at the medium boundary and the energy dependence of both discrete (radiative and photonuclear) and continuous (ionization) muon energy losses, with resonable requirements for the high-energy behavior of the initial spectrum and differential cross sections of the muon-matter interactions. (To be published in the Proceedings of the Second NESTOR International Workshop, 19 -- 21 October 1992, Pylos, Greece.)
dc.descriptionDFF 179/93. REVTeX, 37 pages, no figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9301263
dc.identifierhttp://arxiv.org/abs/hep-ph/9301263
dc.identifierPhysics of Atomic Nuclei 57 (1994) 412-424
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44745
dc.subjectHigh Energy Physics - Phenomenology
dc.titleHigh-Energy Cosmic-Ray Muons Under Thick Layers of Matter I. a Method to Solve the Transport Equation
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