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Probing the energy spectrum of hadrons in proton air interactions at ultrahigh energies through the fluctuations of the muon content of extensive air showers

dc.contributor.authorCazon, Lorenzo
dc.contributor.authorConceição, Ruben
dc.contributor.authorRiehn, Felix
dc.date.accessioned2019-02-05T16:03:36Z
dc.date.available2019-02-05T16:03:36Z
dc.date.issued2018-09-10
dc.date.updated2019-02-05T16:03:35Z
dc.description.abstractWe demonstrate that the shower-to-shower fluctuations of the muon content of extensive air showers correlate with the fluctuations of a variable of the first interaction of Ultra High Energy Cosmic Rays, which is computed from the fraction of energy carried by the hadrons that sustain the hadronic cascade. The influence of subsequent stages of the shower development is found to play a sub-dominant role. As a consequence, the shower-to-shower distribution of the muon content is a direct probe of the hadron energy spectrum of interactions beyond 100 TeV center of mass energies.
dc.description.versionPeer Reviewed
dc.identifierPhys.Lett. B784 (2018) 68-76; DOI 10.1016/j.physletb.2018.07.026
dc.identifier.urihttp://dx.doi.org/10.1016/j.physletb.2018.07.026
dc.identifier.urihttp://hdl.handle.net/10400.26/27596
dc.language.isoeng
dc.titleProbing the energy spectrum of hadrons in proton air interactions at ultrahigh energies through the fluctuations of the muon content of extensive air showers
dc.typejournal article
dspace.entity.typePublication
rcaap.rightsopenAccesspt
rcaap.typearticle

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