用冰立方大气中微子干涉测量法研究中微子振荡中的洛伦兹破坏

B. Skrzypek, C. Arguelles
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引用次数: 0

摘要

洛伦兹不变性是时空的基本对称性,它支撑着标准模型(SM)和我们对粒子物理中高能现象的理解。然而,在量子引力尺度之外,我们期望SM被一个更基本的协变理论所取代,这个协变理论给出了引力的量子描述。由该理论产生的有效理论可以打破洛伦兹不变性,从而预测出表现出洛伦兹违反的低能表现的观测值。特别是,这些观测值可能是对中微子振荡的次要贡献,因此可以解释反常的风味测量。标准模型扩展(SME)形式描述了这样一个有效的理论,它预测的项的特征振荡长度在冰立方中微子天文台可以观测到的大气中微子能量范围内变得显著。我们描述了过去的测量和努力,利用十年的数据以及新的能量重建来研究$\nu_{\mu}$消失。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Lorentz Violation in Neutrino Oscillations Using IceCube Atmospheric Neutrino Interferometry
Lorentz invariance is a fundamental symmetry of spacetime underpinning the Standard Model (SM) and our understanding of high-energy phenomena in particle physics. However, beyond the quantum gravity scale, we expect the SM to be replaced with a more fundamental, covariant theory giving a quantum description of gravity. The effective theory arising from this theory can break Lorentz invariance and thus predicts observables that exhibit low-energy manifestations of Lorentz violation. In particular, these observables could be a subleading contribution to neutrino oscillations and could therefore explain anomalous flavor measurements. The Standard Model Extension (SME) formalism describing such an effective theory predicts terms whose characteristic oscillation length becomes significant at atmospheric neutrino energies accessible by the IceCube Neutrino Observatory. We descibe past measurements and efforts to extend these using ten years of data along with a new energy reconstruction to study $\nu_{\mu}$ disappearance.
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