dc.contributor.author Katori, T en_US dc.date.accessioned 2016-04-13T10:05:40Z dc.date.submitted 2016-04-01T19:49:48.545Z dc.identifier.uri http://qmro.qmul.ac.uk/xmlui/handle/123456789/11803 dc.description 8 pages, 8 figures, Proceedings of the XLIIIrd Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Italy, March 1-8, 2008 dc.description 8 pages, 8 figures, Proceedings of the XLIIIrd Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Italy, March 1-8, 2008 en_US dc.description.abstract Neutrino 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.rights arXiv record: http://arxiv.org/abs/0805.2476 dc.subject hep-ex en_US dc.subject hep-ex en_US dc.title Neutrino Cross Section Measurements for Long-Baseline Accelerator-based Neutrino Oscillation Experiments en_US dc.type Article pubs.author-url http://arxiv.org/abs/0805.2476v1 en_US pubs.notes Not known en_US
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