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Secondary Decays in Atmospheric Charm Contributions to the Flux of Muons and Muon Neutrinos

We present a calculation of the fluxes of muons and muon neutrinos from the decays of pions and kaons that are themselves the decay products of charmed particles produced in the atmosphere by cosmic ray-air collisions. Using the perturbative cross section for charm production, these lepton fluxes ar...

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Detalles Bibliográficos
Autores principales: Pasquali, L, Reno, M H, Sarcevic, I
Lenguaje:eng
Publicado: 1997
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0927-6505(98)00019-X
http://cds.cern.ch/record/336289