类空间粒子的产生:基于马约拉纳方程的解释

L. Nanni
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引用次数: 1

摘要

本文从相对论量子力学的角度,重新考虑了慢子、速子和色子中普通粒子的衰变。Lemke已经从协变运动学的角度研究了这个问题。由于衰变涉及类空粒子和类时粒子,因此该研究使用了任意自旋粒子的马约拉纳方程。该方程描述了大质量粒子的速子和慢子领域,并探讨了类空间粒子如何发展的问题。该方法证实了Lemke理论提供的运动学约束,并证明了一些可能的衰变比其他的更有利。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Space-like Particle Production: An Interpretation Based on the Majorana Equation
This study reconsiders the decay of an ordinary particle in bradyons, tachyons and luxons in the field of the relativistic quantum mechanics. Lemke already investigated this from the perspective of covariant kinematics. Since the decay involves both space-like and time-like particles, the study uses the Majorana equation for particles with an arbitrary spin. The equation describes the tachyonic and bradyonic realms of massive particles, and approaches the problem of how space-like particles might develop. This method confirms the kinematic constraints that Lemke's theory provided and proves that some possible decays are more favorable than others are.
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