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The next generation of neutrino experiments at accelerators aims to establish matter-antimatter asymmetry in neutrino flavor oscillations. Precision oscillation measurements require inference of neutrino fluxes as a function of flavor and energy from the products of O(GeV) neutrino interactions on nuclei.
I’ll discuss some recent results from the MINERvA experiment and how they help with this inference.
https://cern.zoom.us/j/61585612649?pwd=FoLJQF7A3uVaG1ss9JoguyXrFeYHYY.1