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General COHERENT Constraints on Neutrino Non-Standard Interactions

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arxiv 1909.00466 v2 pith:TNNE6M3M submitted 2019-09-01 hep-ph hep-ex

classification hep-phhep-ex
keywords constraintsdowncoherentdataneutrinoobtainedparameterscase
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We present the results of a systematic study of the constraints on neutrino neutral-current non-standard interactions (NSI) that can be obtained from the analysis of the COHERENT spectral and temporal data. First, we consider the general case in which all the ten relevant neutral-current NSI parameters are considered as free. We show that they are very weakly constrained by the COHERENT data because of possible cancellations between the up and down quark contributions. However, the up-down average parameters are relatively well constrained and the strongest constraints are obtained for an appropriate linear combination of up and down NSI parameters. We also consider the case in which there are only NSI with either up or down quarks, and we show that the LMA-Dark fit of solar neutrino data is excluded at $5.6\sigma$ and $7.2\sigma$ respectively, for NSI with up and down quark. We finally present the tight constraints that can be obtained on each NSI parameter if it is the dominant one, assuming that the effects of the others are negligible.

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Forward citations

Cited by 6 Pith papers

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

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  3. Sensitivity study of a sapphire detector using Coherent Elastic Neutrino-Nucleus Scattering process

    hep-ph 2025-02 conditional novelty 5.0 of 10

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    Projected ESS CEνNS measurements would improve current constraints on the weak mixing angle, nuclear neutron radii, and several new physics scenarios by large factors, and would lead in some unexplored mass ranges.

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    hep-ph 2025-10 conditional novelty 4.0 of 10

    Argon CEvNS detectors at stopped-pion sources project sin²θW precision near 1%, neutrino magnetic-moment limits near 10⁻⁹ μB, charge-radius limits near 10⁻³² cm², and vector NSI sensitivity at the 10⁻² level.

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