Phenomenology of the Magueijo-Smolin model of doubly special relativity using the non-relativistic limit of the Dirac equation, spin and Zeeman effect

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Physics Letters B Pub Date : 2025-04-01 Epub Date: 2025-03-05 DOI:10.1016/j.physletb.2025.139364
Ilyas Haouam
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Abstract

In this article, we investigate the phenomenology of the Magueijo-Smolin (MS) model of Doubly Special Relativity by examining the non-relativistic (NR) limit of the Dirac equation and its implications for spin dynamics. A deformed Dirac equation is derived within the MS model framework and is used to explore the continuity equation and the NR limit, leading to a deformed Schrödinger-Pauli equation. The effectiveness of this NR limit is compared to the Foldy–Wouthuysen transformation. Additionally, we obtain the classical limit of the deformed Schrödinger-Pauli equation and evaluate the gyromagnetic factor of the Dirac particle. The spin motion equation and a deformed magnetization current are also derived within the MS model framework. Furthermore, using the mass difference between the tau and anti-tau particles induced by the MS model, we establish a lower bound on the parameter κ. The MS model's impact is analyzed in both relativistic and NR systems through the continuity equation, and the anomalous Zeeman effect is extensively studied in this context. This study highlights the influence of the MS model on both relativistic and NR dynamics.
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利用狄拉克方程、自旋和塞曼效应的非相对论性极限研究双重狭义相对论的Magueijo-Smolin模型的现象学
本文通过考察狄拉克方程的非相对论性极限及其对自旋动力学的影响,研究了双重狭义相对论的Magueijo-Smolin (MS)模型的现象学。在MS模型框架内推导了变形的Dirac方程,并利用该方程对连续性方程和NR极限进行了探讨,得到了变形的Schrödinger-Pauli方程。将该NR极限的有效性与Foldy-Wouthuysen变换进行了比较。此外,我们还得到了变形Schrödinger-Pauli方程的经典极限,并计算了狄拉克粒子的回旋磁因子。在MS模型框架内推导了自旋运动方程和变形磁化电流。此外,利用MS模型诱导的tau粒子和反tau粒子之间的质量差,我们建立了参数κ的下界。通过连续性方程分析了MS模型在相对论和NR系统中的影响,并在此背景下广泛研究了异常塞曼效应。本研究强调了MS模型对相对论和NR动力学的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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