dc.creatorAbreu, P.
dc.creatorAlbuquerque, Ivone Freire da Mota e
dc.creatorSouza, Vitor de
dc.creatorGouffon, Philippe
dc.creatorPeixoto, C. J. Todero
dc.creatorTridapalli, D. B.
dc.creatoret al.
dc.date.accessioned2014-05-27T19:03:02Z
dc.date.accessioned2018-07-04T16:45:30Z
dc.date.available2014-05-27T19:03:02Z
dc.date.available2018-07-04T16:45:30Z
dc.date.created2014-05-27T19:03:02Z
dc.date.issued2013-05
dc.identifierJournal of Cosmology and Astroparticle Physics, Bristol: Institute of Physics - IOP, v. 2013, n. 5, p. 009-1-009-18, May 2013
dc.identifier1475-7516
dc.identifierhttp://www.producao.usp.br/handle/BDPI/45066
dc.identifier10.1088/1475-7516/2013/05/009
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1639962
dc.description.abstractWe derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than ~(0.06 - 5) × '10 POT. -4' 'Mpc POT. -3' at 95% CL, depending on the magnitude of the magnetic deflections. Similar bounds, in the range (0.2 - 7) × '10 POT. -4' 'Mpc POT. -3', were obtained for sources following the local matter distribution.
dc.languageeng
dc.publisherInstitute of Physics - IOP
dc.publisherBristol
dc.relationJournal of Cosmology and Astroparticle Physics
dc.rightsCopytright IOP Publishing Ltd and Sissa Medialab srl
dc.rightsrestrictedAccess
dc.subjectUltra high energy cosmic rays
dc.subjectCosmic ray experiments
dc.titleBounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
dc.typeArtículos de revistas


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