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Consistent QFT description of non-standard neutrino interactions

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arxiv 1910.02971 v3 pith:VWXBMMSB submitted 2019-10-07 hep-ph hep-th

classification hep-phhep-th
keywords interactionsfieldneutrinophysicsstandardtheoryapproachdescription
verification ladder T0 review T1 audit T2 compute T3 formal

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Neutrino oscillations are precision probes of new physics beyond the Standard Model. Apart from neutrino masses and mixings, they are also sensitive to possible deviations of low-energy interactions between quarks and leptons from the Standard Model predictions. In this paper we develop a systematic description of such non-standard interactions (NSI) in oscillation experiments within the quantum field theory framework. We calculate the event rate and oscillation probability in the presence of general NSI, starting from the effective field theory (EFT) in which new physics modifies the flavor or Lorentz structure of charged-current interactions between leptons and quarks. We also provide the matching between the EFT Wilson coefficients and the widely used simplified quantum-mechanical approach, where new physics is encoded in a set of production and detection NSI parameters. Finally, we discuss the consistency conditions for the standard NSI approach to correctly reproduce the quantum field theory result.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Real and Virtual Propagation in Neutrino Oscillations

    hep-ph 2026-06 unverdicted novelty 6.0 of 10

    In Gaussian wave-packet QFT, flavor oscillations switch on only after a propagation-time threshold set by the wave-packet energy uncertainty and the intermediate particle's decay width; below it the neutrino is purely...

  2. From DUNE Sensitivities to UV Models: Implications of Flavour Constraints

    hep-ph 2026-06 conditional novelty 5.0 of 10

    Simple weakly-coupled BSM models cannot produce a DUNE-visible e-tau semileptonic NSI: flavour constraints cap C_lq,1311 at about 1e-2 TeV^-2, nearly an order below DUNE's reach.

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