Superposition of neutrino helicity states creates azimuthal asymmetry in recoil momenta for scattering on electrons, protons, and nuclei, offering a way to observe spin oscillations with directional detection.
Nobel lecture: The sudbury neutrino observatory: Observation of flavor change for solar neutrinos
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Relating two GNI parametrizations shows scalar neutrino-quark interactions are more tightly constrained by COHERENT while tensor interactions are better bounded by deep inelastic scattering.
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The potential of directional neutrino detection to observe neutrino spin oscillations
Superposition of neutrino helicity states creates azimuthal asymmetry in recoil momenta for scattering on electrons, protons, and nuclei, offering a way to observe spin oscillations with directional detection.
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Generalized Neutrino Interactions: constraints and parametrizations
Relating two GNI parametrizations shows scalar neutrino-quark interactions are more tightly constrained by COHERENT while tensor interactions are better bounded by deep inelastic scattering.