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Constraints on hadronic models in extensive air showers with the Pierre Auger Observatory

dc.contributor.authorEspadanal, J.
dc.date.accessioned2019-02-04T11:00:39Z
dc.date.available2019-02-04T11:00:39Z
dc.date.issued2016-11-29
dc.date.updated2019-02-04T11:00:39Z
dc.description.abstractExtensive air showers initiated by ultra-high energy cosmic rays are sensitive to the details of hadronic interactions models, so we present the main results obtained using the data of the Pierre Auger Observatory. The depth at which the maximum of the electromagnetic development takes place is the most sensitive parameter to infer the nature of the cosmic rays. However, the hadronic models cannot describe consistently the maximum and the muon measurements at energies higher than those reached at the LHC.
dc.description.versionPeer Reviewed
dc.identifierEPJ Web Conf. 130 (2016) 07004; DOI 10.1051/epjconf/201613007004
dc.identifier.urihttp://dx.doi.org/10.1051/epjconf/201613007004
dc.identifier.urihttp://hdl.handle.net/10400.26/27167
dc.language.isoeng
dc.titleConstraints on hadronic models in extensive air showers with the Pierre Auger Observatory
dc.typejournal article
dspace.entity.typePublication
rcaap.rightsopenAccesspt
rcaap.typearticle

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