2+1 几何图形的代数分类:一种新方法

M. Papajčı́k, J. Podolský
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引用次数: 0

摘要

我们提出了一种将 2+1 空间划分为 I、II、D、III、N 和 O 类型的代数方法,无需使用任何场方程。该方法基于不同提升权重的纽曼-彭罗斯曲率标量 Psi_A 的 2+1 类比,它们是科顿张量在合适的空三元组上的特定投影。然后,代数类型就简单地由这些科顿张量的逐渐消失决定了,从提升权重最大的科顿张量开始。这种分类与棉花对齐空方向(CAND)的特定多重性和相应的贝尔-德贝弗标准直接相关。利用双向(即 2-形式)分解,我们证明了我们的方法完全等同于基于特征值问题和确定科顿-约克张量各自的典范约旦形式的 2+1 空间的通常彼得罗夫式分类。我们还根据关键的多项式曲率不变式推导出了代数分类的简单综合算法。为了证明我们的方法的实用性,我们对几个明确的例子进行了分类,即具有对齐电磁场和宇宙学常数的罗宾逊-特劳特曼时空的一般类别,以及其他各种代数类型的度量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Algebraic classification of 2+1 geometries: a new approach
We present a convenient method of algebraic classification of 2+1 spacetimes into the types I, II, D, III, N and O, without using any field equations. It is based on the 2+1 analogue of the Newman-Penrose curvature scalars Psi_A of distinct boost weights, which are specific projections of the Cotton tensor onto a suitable null triad. The algebraic types are then simply determined by the gradual vanishing of such Cotton scalars, starting with those of the highest boost weight. This classification is directly related to the specific multiplicity of the Cotton-aligned null directions (CANDs) and to the corresponding Bel-Debever criteria. Using a bivector (that is 2-form) decomposition, we demonstrate that our method is fully equivalent to the usual Petrov-type classification of 2+1 spacetimes based on the eigenvalue problem and determining the respective canonical Jordan form of the Cotton-York tensor. We also derive a simple synoptic algorithm of algebraic classification based on the key polynomial curvature invariants. To show the practical usefulness of our approach, we perform the classification of several explicit examples, namely the general class of Robinson-Trautman spacetimes with an aligned electromagnetic field and a cosmological constant, and other metrics of various algebraic types.
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