Muon and Muon Neutrino Fluxes from Atmospheric Charm

The charm contribution to the atmospheric fluxes of muons and muon neutrinos may be enhanced by as much as a factor of 10 when one includes the contributions of D->pi,K->leptons and folds in uncertainties in the charm cross section and energy distribution. In the energy range considered here,...

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Detalles Bibliográficos
Autores principales: Pasquali, L., Reno, M.H., Sarcevic, I.
Lenguaje:eng
Publicado: 1999
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1016/S0920-5632(98)00452-6
http://cds.cern.ch/record/339418
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author Pasquali, L.
Reno, M.H.
Sarcevic, I.
author_facet Pasquali, L.
Reno, M.H.
Sarcevic, I.
author_sort Pasquali, L.
collection CERN
description The charm contribution to the atmospheric fluxes of muons and muon neutrinos may be enhanced by as much as a factor of 10 when one includes the contributions of D->pi,K->leptons and folds in uncertainties in the charm cross section and energy distribution. In the energy range considered here, from 100 GeV to 10 TeV, the charm contribution is small compared to the conventional flux of muons and muon neutrinos.
id cern-339418
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
record_format invenio
spelling cern-3394182023-03-14T17:00:54Zdoi:10.1016/S0920-5632(98)00452-6http://cds.cern.ch/record/339418engPasquali, L.Reno, M.H.Sarcevic, I.Muon and Muon Neutrino Fluxes from Atmospheric CharmParticle Physics - PhenomenologyThe charm contribution to the atmospheric fluxes of muons and muon neutrinos may be enhanced by as much as a factor of 10 when one includes the contributions of D->pi,K->leptons and folds in uncertainties in the charm cross section and energy distribution. In the energy range considered here, from 100 GeV to 10 TeV, the charm contribution is small compared to the conventional flux of muons and muon neutrinos.The charm contribution to the atmospheric fluxes of muons and muon neutrinos may be enhanced by as much as a factor of 10 when one includes the contributions of D->pi,K->leptons and folds in uncertainties in the charm cross section and energy distribution. In the energy range considered here, from 100 GeV to 10 TeV, the charm contribution is small compared to the conventional flux of muons and muon neutrinos.hep-ph/9711457oai:cds.cern.ch:3394181999
spellingShingle Particle Physics - Phenomenology
Pasquali, L.
Reno, M.H.
Sarcevic, I.
Muon and Muon Neutrino Fluxes from Atmospheric Charm
title Muon and Muon Neutrino Fluxes from Atmospheric Charm
title_full Muon and Muon Neutrino Fluxes from Atmospheric Charm
title_fullStr Muon and Muon Neutrino Fluxes from Atmospheric Charm
title_full_unstemmed Muon and Muon Neutrino Fluxes from Atmospheric Charm
title_short Muon and Muon Neutrino Fluxes from Atmospheric Charm
title_sort muon and muon neutrino fluxes from atmospheric charm
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0920-5632(98)00452-6
http://cds.cern.ch/record/339418
work_keys_str_mv AT pasqualil muonandmuonneutrinofluxesfromatmosphericcharm
AT renomh muonandmuonneutrinofluxesfromatmosphericcharm
AT sarcevici muonandmuonneutrinofluxesfromatmosphericcharm

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