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dc.contributor.authorAguilar-Arevalo, AAen_US
dc.contributor.authorBrown, BCen_US
dc.contributor.authorBugel, Len_US
dc.contributor.authorCheng, Gen_US
dc.contributor.authorChurch, EDen_US
dc.contributor.authorConrad, JMen_US
dc.contributor.authorDharmapalan, Ren_US
dc.contributor.authorDjurcic, Zen_US
dc.contributor.authorFinley, DAen_US
dc.contributor.authorFord, Ren_US
dc.contributor.authorGarcia, FGen_US
dc.contributor.authorGarvey, GTen_US
dc.contributor.authorGrange, Jen_US
dc.contributor.authorHuelsnitz, Wen_US
dc.contributor.authorIgnarra, Cen_US
dc.contributor.authorImlay, Ren_US
dc.contributor.authorJohnson, RAen_US
dc.contributor.authorKaragiorgi, Gen_US
dc.contributor.authorKatori, Ten_US
dc.contributor.authorKobilarcik, Ten_US
dc.contributor.authorLouis, WCen_US
dc.contributor.authorMariani, Cen_US
dc.contributor.authorMarsh, Wen_US
dc.contributor.authorMills, GBen_US
dc.contributor.authorMirabal, Jen_US
dc.contributor.authorMoore, CDen_US
dc.contributor.authorMousseau, Jen_US
dc.contributor.authorNienaber, Pen_US
dc.contributor.authorOsmanov, Ben_US
dc.contributor.authorPavlovic, Zen_US
dc.contributor.authorPerevalov, Den_US
dc.contributor.authorPolly, CCen_US
dc.contributor.authorRay, Hen_US
dc.contributor.authorRoe, BPen_US
dc.contributor.authorRussell, ADen_US
dc.contributor.authorShaevitz, MHen_US
dc.contributor.authorSpitz, Jen_US
dc.contributor.authorStancu, Ien_US
dc.contributor.authorTayloe, Ren_US
dc.contributor.authorWater, RGVDen_US
dc.contributor.authorWhite, DHen_US
dc.contributor.authorWickremasinghe, DAen_US
dc.contributor.authorZeller, GPen_US
dc.contributor.authorZimmerman, EDen_US
dc.date.accessioned2016-04-13T12:56:07Z
dc.date.submitted2016-04-01T15:41:39.500Z
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/11835
dc.description.abstractThis paper explores the use of $L/E$ oscillation probability distributions to compare experimental measurements and to evaluate oscillation models. In this case, $L$ is the distance of neutrino travel and $E$ is a measure of the interacting neutrino's energy. While comparisons using allowed and excluded regions for oscillation model parameters are likely the only rigorous method for these comparisons, the $L/E$ distributions are shown to give qualitative information on the agreement of an experiment's data with a simple two-neutrino oscillation model. In more detail, this paper also outlines how the $L/E$ distributions can be best calculated and used for model comparisons. Specifically, the paper presents the $L/E$ data points for the final MiniBooNE data samples and, in the Appendix, explains and corrects the mistaken analysis published by the ICARUS collaboration.en_US
dc.rightsarXiv record: http://arxiv.org/abs/1407.3304
dc.subjecthep-exen_US
dc.subjecthep-exen_US
dc.subjecthep-phen_US
dc.subjectnucl-exen_US
dc.titleUsing L/E Oscillation Probability Distributionsen_US
dc.typeArticle
pubs.author-urlhttp://arxiv.org/abs/1407.3304v1en_US
pubs.notesNot knownen_US


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