Neutrino Cross Section Measurements for Long-Baseline Accelerator-based Neutrino Oscillation Experiments

dc.creatorKatori, Teppei
dc.date2008-05-16
dc.date.accessioned2026-07-07T09:39:23Z
dc.date.available2026-07-07T09:39:23Z
dc.descriptionNeutrino oscillations are clear evidence for physics beyond the standard model. The goal of next-generation neutrino oscillation experiments is to find a non-zero $θ_{13}$, 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 $Δm^2_{32}$ and $sin^22θ_{23}$, and (2) good background prediction to measure $ν_e$ 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.
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.identifierhttps://arxiv.org/abs/0805.2476
dc.identifierhttp://arxiv.org/abs/0805.2476
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/161152
dc.subjectHigh Energy Physics - Experiment
dc.titleNeutrino Cross Section Measurements for Long-Baseline Accelerator-based Neutrino Oscillation Experiments
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