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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

dc.contributor.authorPierre Auger collaboration (486 authors)
dc.contributor.authorAbreu, Pedro
dc.contributor.authorAndringa, Sofia
dc.contributor.authorAssis, Pedro
dc.contributor.authorBrogueira, Pedro
dc.contributor.authorCazon, Lorenzo
dc.contributor.authorConceição, Ruben
dc.contributor.authorDiogo, Francisco
dc.contributor.authorEspadanal, Joao
dc.contributor.authorGonçalves, Patrícia
dc.contributor.authorOliveira, Micael
dc.contributor.authorPimenta, Mário
dc.contributor.authorSanto, Catarina E
dc.contributor.authorSantos, Eva
dc.contributor.authorSarmento, Raul
dc.contributor.authorTomé, Bernardo
dc.date.accessioned2019-02-04T05:05:04Z
dc.date.available2019-02-04T05:05:04Z
dc.date.issued2015-06-20
dc.date.updated2019-02-04T05:05:04Z
dc.description.abstractEnergy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with $E \ge 6 \times 10^{19}$ eV by analyzing cosmic rays with energies above $E \ge 5 \times 10^{18}$ eV arriving within an angular separation of approximately 15$^{\circ }$ . We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.
dc.description.versionPeer Reviewed
dc.identifierEur.Phys.J. C75 (2015) 269; DOI 10.1140/epjc/s10052-015-3471-0
dc.identifier.urihttp://dx.doi.org/10.1140/epjc/s10052-015-3471-0
dc.identifier.urihttp://hdl.handle.net/10400.26/26697
dc.language.isoeng
dc.titleSearch for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
dc.typejournal article
dspace.entity.typePublication
rcaap.rightsopenAccesspt
rcaap.typearticle

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