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dc.contributor.authorKatori, Ten_US
dc.date.accessioned2016-04-13T10:05:40Z
dc.date.submitted2016-04-01T19:49:48.545Z
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/11803
dc.description8 pages, 8 figures, Proceedings of the XLIIIrd Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Italy, March 1-8, 2008
dc.description8 pages, 8 figures, Proceedings of the XLIIIrd Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Italy, March 1-8, 2008en_US
dc.description.abstractNeutrino oscillations are clear evidence for physics beyond the standard model. The goal of next-generation neutrino oscillation experiments is to find a non-zero $\theta_{13}$, the last mixing matrix element for which we only know an upper limit. For this, next-generation long-baseline neutrino oscillation experiments require an order of magnitude better sensitivities. In particular, accelerator-based experiments such as T2K and NOvA experiments need (1) good neutrino energy reconstruction for the precise measurement of $\Delta m^2_{32}$ and $sin^22\theta_{23}$, and (2) good background prediction to measure $\nu_e$ appearance signals. Current and near future high statistics neutrino experiments, such as K2K, MiniBooNE, SciBooNE, MINOS, and MINERvA help both (1) and (2) by precise signal and background channel measurements.en_US
dc.rightsarXiv record: http://arxiv.org/abs/0805.2476
dc.subjecthep-exen_US
dc.subjecthep-exen_US
dc.titleNeutrino Cross Section Measurements for Long-Baseline Accelerator-based Neutrino Oscillation Experimentsen_US
dc.typeArticle
pubs.author-urlhttp://arxiv.org/abs/0805.2476v1en_US
pubs.notesNot knownen_US
pubs.organisational-group/Queen Mary University of London
pubs.organisational-group/Queen Mary University of London/Faculty of Science & Engineering
pubs.organisational-group/Queen Mary University of London/Faculty of Science & Engineering/Physics and Astronomy


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