分辨中微子振荡中的超标准模型效应

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
A. Calatayud-Cadenillas, A. Pérez-G, A.M. Gago
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引用次数: 0

摘要

我们系统地评估了DUNE实验区分各种超标准中微子振荡假设对组合的能力。对于配对比较,我们评估统计分离,其中一个假设扮演真实信号的角色,而另一个对应于测试信号。研究中的超标准中微子振荡假说包括中微子衰变(不可见和可见)、非标准相互作用、量子退相干和违反等效原理。我们发现,与其他假设相比,违反等效原理是最容易区分的。此外,从我们的χ2统计分离检验中,我们研究了测量到的cp违反相位δCP、θ23和Δm312相对于它们各自的真实值之间的潜在差异,这在给定的比较中可能发生。在我们的分析中,我们将δCP的真实值设为90°和180°,而θ23和Δm312在其全局拟合值中是固定的。特别是,即使在超标准中微子振荡假设的情形在统计上无法区分的情况下,测量值也可能表现出与其真实值的显著偏差。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Distinguishing beyond-standard model effects in neutrino oscillation
We systematically assess the DUNE experiment's ability to distinguish between various beyond-standard neutrino oscillation hypotheses pair combinations. For a pair comparison, we evaluate the statistical separation, where one hypothesis plays the role of the true signal while the other corresponds to the test signal. The beyond-standard neutrino oscillation hypotheses under scrutiny include neutrino decay (invisible and visible), non-standard inter-actions, quantum decoherence, and the violation of the equivalence principle. We found that the violation of the equivalence principle is the easiest to differentiate compared to the rest of the hypotheses. Additionally, from our χ2 statistical separation test, we investigate potential discrepancies between the measured CP-violation phase δCP, θ23, and Δm312 relative to their respective true values, which could occur for a given comparison. In our analysis, we will take the true values of δCP as 90 and 180, while θ23 and Δm312 are fixed in its global fit values. In particular, even in cases where the scenarios of beyond-standard neutrino oscillation hypotheses are statistically indistinguishable, the measured values can exhibit significant deviations from their true values.
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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