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Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

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Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

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dc.contributor.author The Pierre Auger Collaboration
dc.contributor.author Pastor Carpi, Sergio
dc.date.accessioned 2014-02-24T09:05:42Z
dc.date.available 2014-05-09T09:05:42Z
dc.date.issued 2013
dc.identifier.citation Pierre Auger Observatory Pastor Carpi, Sergio 2013 Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory Journal Of Cosmology And Astroparticle Physics 1305 05 009-1 009-18
dc.identifier.uri http://hdl.handle.net/10550/33248
dc.description.abstract We 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 similar to (0.06 - 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 - 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.
dc.relation.ispartof Journal Of Cosmology And Astroparticle Physics, 2013, vol. 1305, num. 05, p. 009-1-009-18
dc.subject Astronomia
dc.subject Cosmologia
dc.title Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
dc.type journal article es_ES
dc.date.updated 2014-02-24T09:05:42Z
dc.identifier.doi 10.1088/1475-7516/2013/05/009
dc.identifier.idgrec 093582
dc.rights.accessRights open access es_ES
dc.identifier.url 10.1088/1475-7516/2013/05/009

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