关于Kerr-NUT时空的正则化。我

G. Nashed
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引用次数: 2

摘要

在广义相对论的遥平行等效(TEGR)理论框架内,采用与坐标无关的引力能量-动量和黎曼连接1-形式e Γ β α两种方法计算了Kerr-NUT时空的总能量和动量。结果表明,这两种方法得到的结果都是不可接受的,即值是发散的。因此,我们提出了一种局部洛伦兹变换,它起到了正则化工具的作用,可以在不扭曲真实引力贡献的情况下减去惯性效应。这种变换使得到的时空保持为TEGR运动方程的解。学科索引:451,453
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On the Regularization of Kerr-NUT Spacetime. I
Within the framework of teleparallel equivalent of general relativity (TEGR) theory, calculation of the total energy and momentum of Kerr-NUT spacetimes have been employed using two methods of the gravitational energy-momentum, which is coordinate independent, and the Riemannian connection 1-form, e Γ β α . It has been shown that the two methods give the same unacceptable result, i.e., divergent value. Therefore, a local Lorentz transformation that plays a role of a regularizing tool, which subtracts the inertial effects without distorting the true gravitational contribution, has been suggested. This transformation keeps the resulting spacetime to be a solution of the equations of motion of TEGR. Subject Index: 451, 453
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来源期刊
Progress of Theoretical Physics
Progress of Theoretical Physics 物理-物理:综合
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