2018
DOI: 10.5281/zenodo.1228631
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Coherent Collaboration Data Release From The First Observation Of Coherent Elastic Neutrino-Nucleus Scattering

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Cited by 27 publications
(29 citation statements)
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“…Coherent elastic neutrino-nucleon scattering (CEνNS) is an allowed standard model (SM) process which was predicted in the seventies [1,2] and was observed very recently by the COHERENT experiment [3][4][5]. In between the theoretical prediction and its observation, the formalism to use CEνNS as a probe for new neutrino physics, new neutral current physics or nuclear physics was pointed out for several scenarios [6][7][8][9][10][11][12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…Coherent elastic neutrino-nucleon scattering (CEνNS) is an allowed standard model (SM) process which was predicted in the seventies [1,2] and was observed very recently by the COHERENT experiment [3][4][5]. In between the theoretical prediction and its observation, the formalism to use CEνNS as a probe for new neutrino physics, new neutral current physics or nuclear physics was pointed out for several scenarios [6][7][8][9][10][11][12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 99%
“…Neutrinos are provided from pions decaying at rest, which in turn are produced from the spallation neutron source. The data we will use in this paper was collected with a total number of 1.76 × 10 23 of protons on target (pot) delivered to liquid mercury [3][4][5]. Monoenergetic muon neutrinos (ν µ ) at E ν = 29.8 MeV are produced isotropically from pion decay at rest (π + → µ + ν µ ) followed by a delayed isotropic flux of electron neutrinos (ν e ) and muon anti-neutrinos (ν µ ) produced subsequently by muon-decay at rest (µ + → ν e e + νµ ).…”
Section: Introductionmentioning
confidence: 99%
“…Here α (β) is the nuisance parameters for the signal rate (the beam-on background) with an uncertainty of σ α = 0.28 (σ β = 0.25) [1]. The statistical uncertainty per energy bin is given by σ i stat = N i meas + 2B i SS + B i on with B i SS being the steady-state background from the anti-coincident data, and B i on the beam-on background mainly from prompt neutrons [48]. To obtain the bounds on the simplified neutrino model, we first set g χL = g χR = g χ and m Z = 10m χ or 2m χ for both case A and B, and scan over possible values of the product of the coefficients g χ g q for a given m χ .…”
Section: Numerical Resultsmentioning
confidence: 99%
“…The first, steady state backgrounds, are present in both beam-on and beamoff data and may be handled using prescribed methods of background subtraction as described in Refs. [4,13]. The second, beam-related-neutrons (BRN) and neutrinoinduced-neutrons (NIN) occur in time with the SNS beam and are hence more difficult to separate.…”
Section: A Backgroundsmentioning
confidence: 99%
“…We build upon the method introduced in Ref. [34] to compare the combined observations [13,35] of the COHER-ENT Collaboration from both CsI(2017) as well as the Ar (CENNS10) detectors with the CEνNS prediction in both non-SUSY and SUSY L µ − L τ models in a likelihood maximization test. We also use the announced total count from the CsI(2020) data in conjunction with that from the Ar detector in a chi-square deviation test of the FIG.…”
Section: Introductionmentioning
confidence: 99%