标题: 微中子震荡与罗伦兹破坏
Neutrino Oscillations and Lorentz Violation
作者: 吴瑜澄
林贵林
邱绍玄
Wu, Yu-Chen
Lin, Guey-Lin
Chiu, Shao-Hsuan
物理研究所
关键字: 微中子;微中子震荡;罗伦兹破坏;罗伦兹对称;震荡;粒子物理;neutrino oscillation;neutrino;Lorentz violation;Lorentz symmetry;oscillation;Particle Physics
公开日期: 2017
摘要: 在微中子震荡的理论中,对于只有两种风味微中子的情况,物质效应可以被精确的解出来。系统中的微中子混合角可以被重新定义之外,微中子震荡机率也可以透过震荡方程式计算。但在标准模型下(Standard Model)有三种风味的微中子,在这种情况下,物质效应无法被我们写下像是两种风味微中子一样的简洁方程式去重新定义三个混合角与震荡机率。
在粒子物理与广义相对论里,罗伦兹对称是一个基础的对称。但有一些弦论(String Theory)的模型中,预测这个对称可能可以被破坏。若有罗伦兹对称被破坏,它会在微中子震荡的汉米尔顿函数(Hamiltonian)中加入一些罗伦兹对称破坏参数。而且微中子震荡被认为是一项强而有力的工具去探索罗伦兹对称破坏效应。
为了了解物质效应与罗伦兹对称破坏如何影响本征值、混合矩阵与震荡机率,我们发展出了一套新的近似理论,当我们考虑到物质效应与罗伦兹对称破坏时用来计算本征值、混合矩阵与震荡机率。透过这个方法我们发现到在低能量情况时,加入物质效应与罗伦兹对称破坏参数将会影响每一个混合角。而在高能量微中子的极限与主导的情况下,我们所得到的第二阶震荡机率跟使用复杂费时的公式计算近似结果是一模一样的。
In the theory of neutrino oscillations, matter effect in two-flavor neutrino situation has been solved exactly. The mixing angle can be redefined and oscillation probability can be calculated by exact formulas. However, there are three flavor neutrinos in Standard Model. Under this circumstance, we can no longer write down elegant formulas to redefine three mixing angles or calculate oscillation probabilities for matter effect solutions.
Lorentz symmetry, a fundamental symmetry in particle physics and general theory of relativity, could be broken at or below the Plank scale as predicted by some string models. This Lorentz violation phenomenon would contribute some Lorentz violation parameters to the Hamiltonian of neutrino oscillations. Neutrino oscillation is regarded as a powerful tool to probe the Lorentz violation.
To understand how matter effect and Lorentz violation parameters affect the eigenvalues, mixing matrix and oscillation probabilities, we develop a new approximation method to calculate these terms when we consider matter effect and Lorentz violation. Through this new expansion, we find that adding matter effect and Lorentz violation effect would make a change on all three mixing angles at low energy scale. While in the case of ultra-high-energy limit and dominance, the second order approximation of probabilities we obtaining is the same as the equations calculated by solution formulas that are more tedious and time consuming.
URI: http://etd.lib.nctu.edu.tw/cdrfb3/record/nctu/#GT070352735
http://hdl.handle.net/11536/140421
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