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Upper limit on the diffuse flux of UHE tau neutrinos from the Pierre Auger Observatory

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Upper limit on the diffuse flux of UHE tau neutrinos from the Pierre Auger Observatory

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dc.contributor.author The Pierre Auger Collaboration
dc.contributor.author Pastor Carpi, Sergio
dc.contributor.author Pinto, Teguayco
dc.date.accessioned 2015-10-27T08:49:07Z
dc.date.available 2015-10-27T08:49:07Z
dc.date.issued 2008
dc.identifier.citation The Pierre Auger Collaboration Pastor Carpi, Sergio Pinto, Teguayco 2008 Upper limit on the diffuse flux of UHE tau neutrinos from the Pierre Auger Observatory Physical Review Letters 100 21 211101-1 211101-7
dc.identifier.uri http://hdl.handle.net/10550/47917
dc.description.abstract The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth¿s crust. Tau leptons from ντ charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January 2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of ντ at EeV energies. Assuming an E−2ν differential energy spectrum the limit set at 90% C.L. is E2νdNντ/dEν<1.3×10−7  GeV cm−2 s−1 sr−1 in the energy range 2×1017  eV<Eν<2×1019  eV.
dc.language.iso eng
dc.relation.ispartof Physical Review Letters, 2008, vol. 100, num. 21, p. 211101-1-211101-7
dc.subject Física
dc.title Upper limit on the diffuse flux of UHE tau neutrinos from the Pierre Auger Observatory
dc.type journal article es_ES
dc.date.updated 2015-10-27T08:49:07Z
dc.identifier.doi 10.1103/PhysRevLett.100.211101
dc.identifier.idgrec 047920
dc.rights.accessRights open access es_ES

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