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Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory

dc.contributor.authorPierre Auger collaboration (464 authors)
dc.contributor.authorAbreu, Pedro
dc.contributor.authorAndringa, Sofia
dc.contributor.authorAssis, Pedro
dc.contributor.authorBlanco, Alberto
dc.contributor.authorBrogueira, Pedro
dc.contributor.authorCazon, Lorenzo
dc.contributor.authorConceição, Ruben
dc.contributor.authorDiogo, Francisco
dc.contributor.authorEspadanal, Joao
dc.contributor.authorLopes, Luis
dc.contributor.authorPimenta, Mário
dc.contributor.authorSantos, Eva
dc.contributor.authorSarmento, Raul
dc.contributor.authorTomé, Bernardo
dc.date.accessioned2019-02-04T06:44:58Z
dc.date.available2019-02-04T06:44:58Z
dc.date.issued2015-05-26
dc.date.updated2019-02-04T06:44:58Z
dc.description.abstractNeutrinos in the cosmic ray flux with energies near 1 EeV and above are detectable with the Surface Detector array (SD) of the Pierre Auger Observatory. We report here on searches through Auger data from 1 January 2004 until 20 June 2013. No neutrino candidates were found, yielding a limit to the diffuse flux of ultrahigh energy neutrinos that challenges the Waxman-Bahcall bound predictions. Neutrino identification is attempted using the broad time structure of the signals expected in the SD stations, and is efficiently done for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for “Earth-skimming” neutrino interactions in the case of tau neutrinos. In this paper the searches for downward-going neutrinos in the zenith angle bins 60°–75° and 75°–90° as well as for upward-going neutrinos, are combined to give a single limit. The 90% C.L. single-flavor limit to the diffuse flux of ultrahigh energy neutrinos with an E-2 spectrum in the energy range 1.0×1017  eV–2.5×1019  eV is Eν2dNν/dEν<6.4×10−9  GeV cm−2 s−1 sr−1.
dc.description.versionPeer Reviewed
dc.identifierPhys.Rev. D91 (2015) 092008; DOI 10.1103/PhysRevD.91.092008
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.91.092008
dc.identifier.urihttp://hdl.handle.net/10400.26/26833
dc.language.isoeng
dc.titleImproved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory
dc.typejournal article
dspace.entity.typePublication
rcaap.rightsopenAccesspt
rcaap.typearticle

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