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Statistical treatment of detection cross-section uncertainties in the analysis of solar neutrino data
High Energy Physics - Phenomenology · Submitted 2 Jun 2000
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We show that the resulting allowed regions for the neutrino oscillation parameters are significantly larger than the ones obtained with uncorrelated uncertainties.
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The abstract, sentence by sentence
We propose a modification to the standard statistical treatment of the detection cross-section uncertainties in the analysis of solar neutrino data. We argue that the uncertainties of the energy-averaged cross sections of the different neutrino fluxes in the same experiment should be treated as correlated. We show that the resulting allowed regions for the neutrino oscillation parameters are significantly larger than the ones obtained with uncorrelated uncertainties.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We propose a modification to the standard statistical treatment of the detection cross-section uncertainties in the analysis of solar neutrino data. | contribution 1.00 | 0.74 | 0.06 | asserted 0.86 |
| s1 | We argue that the uncertainties of the energy-averaged cross sections of the different neutrino fluxes in the same experiment should be treated as correlated. | contribution 0.60 | 0.32 | 0.16 | asserted 0.88 |
| s2 | We show that the resulting allowed regions for the neutrino oscillation parameters are significantly larger than the ones obtained with uncorrelated uncertainties. | result 1.00 | 0.94 | 0.80 | asserted 1.00 |
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The paper
Original abstract
We propose a modification to the standard statistical treatment of the detection cross-section uncertainties in the analysis of solar neutrino data. We argue that the uncertainties of the energy-averaged cross sections of the different neutrino fluxes in the same experiment should be treated as correlated. We show that the resulting allowed regions for the neutrino oscillation parameters are significantly larger than the ones obtained with uncorrelated uncertainties.
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2 arXiv papers cite this in 2 sentences
Papers citing it · 1 sentence without a confident label
Uses its method or tool 1 paper
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The covariance error matrix $V_S$ takes into account the correlations of theoretical uncertainties, according to the discussions in Refs. [ref] .
Bayesian Constraints on theta_{13} from Solar and KamLAND Neutrino Data · $χ^2$ Analysis · 0.83
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