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A semiclassical description of relativistic spin without the use of Grassmann variables and the Dirac equation

机译:不使用格拉斯曼变量和狄拉克方程的相对论自旋的半经典描述

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摘要

We propose a relativistic particle model without Grassmann variables which, being canonically quantized, leads to the Dirac equation. Both Γ-matrices and the relativistic spin tensor are produced through the canonical quantization of the classical variables which parametrize the properly constructed relativistic spin surface. Although there is no mass-shell constraint in our model, our particle's speed cannot exceed the speed of light. The classical dynamics of the model is in correspondence with the dynamics of mean values of the corresponding operators in the Dirac theory. In particular, the position variable experiences Zitterbewegung in noninteracting theory. The classical equations for the spin tensor are the same as those of the Barut-Zanghi model of a spinning particle.
机译:我们提出了一个没有格拉斯曼变量的相对论粒子模型,对它进行了规范化量化,从而得出狄拉克方程。 Γ矩阵和相对论自旋张量都是通过经典变量的规范化量化而产生的,这些经典变量参数化了正确构造的相对论自旋表面。尽管我们的模型中没有质壳约束,但是粒子的速度不能超过光速。该模型的经典动力学与狄拉克理论中相应算子平均值的动力学相对应。尤其是,位置变量在非交互理论中经历了Zitterbewegung。自旋张量的经典方程与旋转粒子的Barut-Zanghi模型的方程相同。

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