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The contribution of charm to high energy atmospheric neutrinos
We discuss the perfomance of the new version of the Sibyll hadronic interaction model Sibyll 2.xx which corrects some of the problems of Sibyll 2.1 and also generates charm hadrons and thus produces very high energy atmospheric neutrinos.
| Autores principales: | , , , , |
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| Lenguaje: | eng |
| Publicado: |
2015
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1016/j.nuclphysbps.2015.06.071 http://cds.cern.ch/record/2159169 |