2017
DOI: 10.1103/physrevd.96.115007
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COHERENT enlightenment of the neutrino dark side

Abstract: In the presence of non-standard neutrino interactions (NSI), oscillation data are affected by a degeneracy which allows the solar mixing angle to be in the second octant (aka the dark side) and implies a sign flip of the atmospheric mass-squared difference. This leads to an ambiguity in the determination of the ordering of neutrino masses, one of the main goals of the current and future experimental neutrino program. We show that the recent observation of coherent neutrino-nucleus scattering by the COHERENT ex… Show more

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Cited by 152 publications
(204 citation statements)
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“…In our previous work [28] we performed a fit to COHERENT data using the available information at that time, which included only the total event rates observed. Last year the collaboration released publicly both the energy and timing information of the events [35].…”
Section: Implementation Of the Coherent Experimentsmentioning
confidence: 99%
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“…In our previous work [28] we performed a fit to COHERENT data using the available information at that time, which included only the total event rates observed. Last year the collaboration released publicly both the energy and timing information of the events [35].…”
Section: Implementation Of the Coherent Experimentsmentioning
confidence: 99%
“…As discussed in Refs. [22,26,[28][29][30], non-oscillation data (such as those collected by neutrino scattering experiments) is needed to break this degeneracy. However, for light enough mediators (M med O(10) GeV) bounds from deep inelastic neutrino scattering experiments, such as CHARM [31] and NuTeV [32], can be successfully avoided [12,26,29].…”
Section: Introductionmentioning
confidence: 99%
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“…Using neutrinos from a stopped pion beam and a 14.6 kg CsI[Na] target, Coherent measured a best-fit count of 134 AE 22 CEνNS events, well in excess of the expected backgrounds. The measured rate was found to be 77 AE 16% of the standard model (SM) prediction, and constrains NSI for some terms more strongly than previous deep inelastic scattering and oscillation experiments [1][2][3]. Properties of the neutron distribution may also be extracted from the measurement [4], and within certain frameworks, models for light dark matter can be probed [5].…”
Section: Introductionmentioning
confidence: 99%
“…We further take an uncertainty of 5% on the experimental background reported by Coherent over the relevant recoil energy range. We note that previous studies of NSI using the Coherent experiment [2,3,16,23] have instead assumed that the per-flavor flux can be identified through a combination of timing and spectral signatures, which would appear to be a reasonable future expectation.…”
Section: A Coherentmentioning
confidence: 99%