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On the Existence and Utility of Rigid Quasilocal Frames

机译:刚性拟局部框架的存在性与效用

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The notion of a rigid quasilocal frame (RQF) provides a geometrically natural way to define a system in general relativity, and a new way to analyze the problem of motion. An RQF is defined as a two-parameter family of timelike worldlines comprising the boundary (topologically ? x S~2) of the history of a finite spatial volume, with the rigidity conditions that the congruence of worldlines be expansion- and shear-free. In other words, the size and shape of the system do not change. In previous work, such quasilocally defined systems in Minkowski space were shown to admit precisely the same six degrees of freedom of rigid body motion that we are familiar with in Newtonian space-time, without any constraints, circumventing a century-old theorem due to Herglotz and Noether. This surprising result is a consequence of the fact that any two-surface with S~2 topology always admits precisely six conformal Killing vectors, which generate an action of the Lorentz group on the sphere. Several representative examples of RQFs were constructed, including one that provides a quasilocal resolution to the Ehrenfest paradox, also a century old. Here we review the previous work in flat spacetime and extend it in three direc- tions: (1) Using a Fermi normal coordinates approach, we explicitly construct, to the first few orders in powers of areal radius, the general solution to the RQF rigidity equations in a generic curved spacetime, and show that the resulting RQFs possess exactly the same six motional degrees of freedom as in flat spacetime; (2) We discuss how RQFs provide a natural context in which to understand the flow of energy, momentum and angular momentum into and out of a system; in particular, we derive a simple, exact expression for the flux of gravitational energy (a gravitational analogue of the Poynting vector) across the boundary of an RQF in terms of operationally-defined geometrical quantities on the boundary; (3) We use this new gravitational (or "geomet- rical")energy flux to resolve another paradox, this one involving electromagnetism in flat spacetime, a paradox we discovered in the course of this work.
机译:刚性准局部框架(RQF)的概念为定义广义相对论的系统提供了一种几何上自然的方式,并且为分析运动问题提供了一种新的方式。 RQF定义为两参数族的时空世界线,包括有限空间体积历史的边界(拓扑上为?x S〜2),其刚性条件是世界线的全等是无扩展和无剪切的。换句话说,系统的大小和形状不会改变。在先前的工作中,这种在Minkowski空间中的准局部定义的系统被证明可以精确地接受我们在牛顿时空中所熟悉的刚体运动的六个自由度,而没有任何限制,从而规避了一个由Herglotz提出的具有百年历史的定理。和Noether。这一令人惊讶的结果是以下事实的结果:任何具有S〜2拓扑的两个表面都始终精确地允许六个共形的杀伤矢量,这些矢量在球上产生了洛伦兹族的作用。构造了RQF的几个代表性示例,其中一个示例为Ehrenfest悖论提供了准局部分辨率,这也已有一个世纪的历史了。在这里,我们回顾一下以前在平面时空上的工作,并将其扩展到三个方向:(1)使用费米法线坐标方法,我们将以面半径为幂的前几个阶显式构造RQF刚度的一般解一般弯曲时空中的方程,表明所得RQF具有与平面时空完全相同的六个运动自由度; (2)我们讨论RQF如何提供一个自然的背景,以便理解能量,动量和角动量流入和流出系统的过程;特别是,我们根据边界上的可操作定义的几何量,得出了跨越RQF边界的重力能量通量(Poynting矢量的重力类似物)的简单精确表达式; (3)我们使用这种新的引力(或“地学”)能量通量来解决另一个悖论,它涉及到在平时空中的电磁现象,这是我们在工作过程中发现的一个悖论。

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