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Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem

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Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem

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dc.contributor.author González García, Mª Concepción
dc.contributor.author Peña Garay, Carlos
dc.contributor.author Smirnov, Alexei Yu
dc.date.accessioned 2014-11-04T11:20:57Z
dc.date.available 2014-11-04T11:20:57Z
dc.date.issued 2001
dc.identifier.citation González García, Mª Concepción Peña Garay, Carlos Smirnov, Alexei Yu 2001 Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem Physical Review D 63 11 113004
dc.identifier.uri http://hdl.handle.net/10550/39580
dc.description.abstract We have performed a detailed study of the zenith angle dependence of the regeneration factor and distributions of events at SNO and SK for different solutions of the solar neutrino problem. In particular, we discuss the oscillatory behavior and the synchronization effect in the distribution for the LMA solution, the parametric peak for the LOW solution, etc. A physical interpretation of the effects is given. We suggest a new binning of events which emphasizes the distinctive features of the zenith angle distributions for the different solutions. We also find the correlations between the integrated day-night asymmetry and the rates of events in different zenith angle bins. The study of these correlations strengthens the identification power of the analysis.
dc.language.iso eng
dc.relation.ispartof Physical Review D, 2001, vol. 63, num. 11, p. 113004
dc.subject Física
dc.title Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem
dc.type journal article es_ES
dc.date.updated 2014-11-04T11:20:57Z
dc.identifier.doi 10.1103/PhysRevD.63.113004
dc.identifier.idgrec 097464
dc.rights.accessRights open access es_ES

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