Uncertainty principle for proper time and mass II

dc.creatorKudaka, Shoju
dc.creatorMatsumoto, Shuichi
dc.date1999-01-14
dc.date1999-01-20
dc.date.accessioned2026-07-07T06:16:03Z
dc.date.available2026-07-07T06:16:03Z
dc.descriptionWhen we quantize a system consisting of a single particle, the proper time $τ$ and the rest mass $m$ are usually dealt with as parameters. In the present article, however, we introduce a new quantization rule by which these quantities are regarded as operators in addition to the position and the momentum. Applying this new rule to a scalar particle and to a particle with spin $ 1/2 $, we analyze the time evolution of the operator $τ$. In the former case, the evolution of the proper time perfectly matches several well-established classical formulae. In the case of the particle with spin 1/2, our new rule implies that an oscillation appears in the time evolution of the operator $τ$. This oscillation is similar to Zitterbewegung which is well-known in the ordinary Dirac theory. We formulate one physical effect of this oscillation by considering the interaction with a gravitational field, and estimate how small it is.
dc.description15 pages, LaTex
dc.identifierhttps://arxiv.org/abs/quant-ph/9901031
dc.identifierhttp://arxiv.org/abs/quant-ph/9901031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/93942
dc.subjectQuantum Physics
dc.titleUncertainty principle for proper time and mass II
dc.typetext

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