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The hadronic interaction model Sibyll-2.3c and inclusive lepton fluxes

dc.contributor.authorAnatoli Fedynitch
dc.contributor.authorFelix Riehn
dc.contributor.authorRalph Engel
dc.contributor.authorThomas K. Gaisser
dc.contributor.authorTodor Stanev
dc.date.accessioned2020-11-06T14:29:58Z
dc.date.available2020-11-06T14:29:58Z
dc.date.issued2018-06-11
dc.description.abstractMuons and neutrinos from cosmic ray interactions in the atmosphere originate from decays of mesons in air-showers. Sibyll-2.3c aims to give a precise description of hadronic interactions in the relevant phase space for conventional and prompt leptons in light of new accelerator data, including that from the LHC. Sibyll is designed primarily as an event generator for use in simulation of extensive air showers. Because it has been tuned for forward physics as well as the central region, it can also be used to calculate inclusive fluxes. The purpose of this paper is to describe the use of Sibyll-2.3c for calculation of fluxes of atmospheric leptons.pt_PT
dc.description.versioninfo:eu-repo/semantics/publishedVersionpt_PT
dc.identifier.doi10.1103/PhysRevD.100.103018pt_PT
dc.identifier.urihttp://hdl.handle.net/10400.26/33960
dc.language.isoengpt_PT
dc.titleThe hadronic interaction model Sibyll-2.3c and inclusive lepton fluxespt_PT
dc.typejournal article
dspace.entity.typePublication
oaire.citation.issue10pt_PT
oaire.citation.titlePhys. Rev. D 100, 103018 (2019)pt_PT
oaire.citation.volume100pt_PT
rcaap.rightsopenAccesspt_PT
rcaap.typearticlept_PT

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