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Particle physics measurements at the highest energies with the Pierre Auger Observatory

dc.contributor.authorAndringa, Sofia
dc.date.accessioned2019-02-04T03:10:47Z
dc.date.available2019-02-04T03:10:47Z
dc.date.issued2014
dc.date.updated2019-02-04T03:10:47Z
dc.description.abstractThe Pierre Auger Observatory measures cosmic rays with energies between 10 17 . 5 eV and 10 20 eV, based on air shower sampling at ground, complemented with shower development measurements with a smaller duty-cycle. The cross-section for the primary interaction of 10 18 eV protons with air has been measured by analysing the maximum of shower development in the atmosphere. This corresponds to a centre-of-mass energy of 57 TeV, and the LHC results show the same evolution of the proton-proton cross-section at intermediate energies. The depth of shower maximum is sensitive to cross-section and primary mass. Its energy evolution indicates a change towards the behavior expected for heavier primaries or larger cross-sections. We will show also the results on other observables related to primary nuclear mass composition.
dc.description.versionPeer Reviewed
dc.identifierPoS EPS-HEP2013 (2013) 391; DOI 10.22323/1.180.0391
dc.identifier.urihttp://dx.doi.org/10.22323/1.180.0391
dc.identifier.urihttp://hdl.handle.net/10400.26/26567
dc.language.isoeng
dc.titleParticle physics measurements at the highest energies with the Pierre Auger Observatory
dc.typejournal article
dspace.entity.typePublication
rcaap.rightsopenAccesspt
rcaap.typearticle

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