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引力拓扑项的类约化及相关螺旋度密度

Spacelike reduction of the gravitational topological terms and associated helicity densities

Hongxi Huang, Jiang Long, Gan Zhao, Xin-Hao Zhou

arXiv 2608.30154首次发表:更新:

发表机构

School of Physics, Huazhong University of Science and Technology(华中科技大学物理学院)

机构由 AI 辅助整理,请以论文原文为准。

AI 中文总结

本研究将引力的Pontryagin和Nieh-Yan拓扑项约化为类空超曲面,经SVT分解得到四种螺旋度密度,研究其展开并应用于多种引力模型。

AI 中文摘要

引力中的螺旋度是一个多面概念,文献中存在若干不等价定义。本研究将拓扑Pontryagin项和Nieh-Yan项约化为恒定时间类空超曲面。值得注意的是,在线性水平应用SVT分解后,我们得到四种不同的螺旋度密度:源自Nieh-Yan项的螺旋度密度,根据其源自矢量模式还是张量模式,被称为自旋1和自旋2的引力磁性螺旋度密度;源自Pontryagin项的螺旋度密度,根据相应的模式贡献,被称为自旋1和自旋2的引力电流螺旋度密度。我们研究了这些螺旋度泛函的模式和多极展开,并将其应用于领头阶牛顿两体系统、弱场 boosted Kerr、局域定义的慢变gyratonic pp-波模型以及线性化引力Hopfion。

英文摘要

Helicity in gravity is a multifaceted concept, and several inequivalent definitions exist in the literature. In this work, we reduce the topological Pontryagin and Nieh-Yan terms to a constant time spacelike hypersurface. Remarkably, upon applying the SVT decomposition at the linearized level, we obtain four distinct helicity densities. The helicity density arising from the Nieh-Yan term is termed the spin-1 and spin-2 gravitomagnetic helicity density, depending on whether it originates from vector or tensor modes. Meanwhile, the helicity density arising from the Pontryagin term is termed the spin-1 and spin-2 gravito-current helicity density, according to the corresponding mode contributions. We study the mode and multipole expansions of these helicity functionals and apply them to leading order Newtonian two-body systems, weak field boosted Kerr, a locally defined slowly varying gyratonic pp-wave model, and a linearized gravitational Hopfion.

Comments54 pages, 3 figures

论文原文

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