Current long-baseline neutrino oscillation experiments (T2K and NOvA) measure oscillation parameters by comparing the evolution of the flavor composition in a pure (anti-)neutrino beam. The oscillation probability evolves as a function of neutrino energy. However, the neutrino energy spectrum measured in these experiments is also determined by the neutrino flux, detector efficiency effects, and the cross-section of neutrino interactions with the target nuclei. The latter introduce sources of systematic uncertainty, whose mis-modelling can severely bias neutrino oscillation parameter measurements. Of the three, the physics of neutrino interactions with matter represents the dominant source of systematic uncertainty.
This seminar will illustrate the mechanisms through which neutrino-nucleus interactions affect neutrino oscillation measurements in current and future long-baseline experiments. Next-generation experiments, such as Hyper-Kamiokande and DUNE, are being developed with extremely ambitious precision physics goals. If kept at current levels, neutrino-nucleus interaction systematic uncertainties will quickly become the limiting factor to their physics programs. This talk will present an overview of experimental and theoretical programs aimed at mitigating these uncertainties as neutrino physics enters the precision measurement era.