Tetiana Kozynets, Philipp Eller, Alan Zander, Manuel Ettengruber, D. Jason Koskinen
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引用次数: 0
Abstract
While the origin of neutrino masses remains unknown, several key neutrino mass generation models result in a non-unitary three-neutrino mixing matrix. To put such models to test, the deviations of the mixing matrix from unitarity can be measured directly through neutrino oscillation experiments. In this study, we perform a Bayesian analysis of the non-unitary mixing model using the recent public data from atmospheric and reactor neutrino experiments — namely IceCube-DeepCore, Daya Bay, and KamLAND. The novelty of our approach compared to the preceding global fits for non-unitarity is in the detailed treatment of the atmospheric neutrino data, which for the first time includes the relevant flux and detector systematic uncertainties. From the Bayesian posteriors on the individual mixing matrix elements, we derive the non-unitarity constraints in the form of normalisations and closures of the mixing matrix rows and columns, assuming either a fully unconstrained matrix or a physically motivated submatrix scenario. We find comparable constraints for electron and tau row normalisations as other similar studies in literature, and additionally reveal strong correlations between muon and tau row constraints induced by the atmospheric systematic uncertainties. We find that the current data is well described by both unitary and non-unitary mixing models, with a strong preference for the unitary mixing indicated by the Bayes factor. With the upcoming IceCube-Upgrade and JUNO detectors, both featuring superior energy resolution compared to the current atmospheric and reactor neutrino experiments, our constraints on the row normalisations in the submatrix case are expected to improve by 25%, 40%, and 20% in the electron, muon, and tau sectors respectively. In the future, our approach can be expanded to include solar and long-baseline neutrino experiments, with the aim to provide more stringent constraints while keeping track of the nuisance parameters that may be degenerate with non-unitarity.
虽然中微子质量的起源仍然未知,但几个关键的中微子质量产生模型导致了一个非酉的三中微子混合矩阵。为了验证这些模型,可以通过中微子振荡实验直接测量混合矩阵与一致性的偏差。在本研究中,我们使用最近来自大气和反应堆中微子实验(即IceCube-DeepCore, Daya Bay和KamLAND)的公开数据对非单一混合模型进行了贝叶斯分析。与之前的非统一全局拟合相比,我们的方法的新颖之处在于对大气中微子数据的详细处理,这是第一次包括相关通量和探测器系统不确定性。从单个混合矩阵元素的贝叶斯后验中,我们以混合矩阵行和列的归一化和闭包的形式推导出非统一性约束,假设一个完全无约束的矩阵或一个物理动机的子矩阵场景。我们发现电子和tau行归一化的约束与文献中其他类似的研究类似,并且还揭示了由大气系统不确定性引起的μ子和tau行约束之间的强相关性。我们发现,目前的数据可以很好地用单一和非单一混合模型来描述,并且对贝叶斯因子所表示的单一混合有强烈的偏好。与目前的大气和反应堆中微子实验相比,即将到来的冰立方升级和朱诺探测器都具有更高的能量分辨率,我们对子矩阵情况下行归一化的限制预计将分别在电子、μ子和tau领域提高25%、40%和20%。在未来,我们的方法可以扩展到包括太阳和长基线中微子实验,目的是提供更严格的约束,同时跟踪可能因非统一性而退化的干扰参数。
期刊介绍:
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