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Electromagnetic-like boost transformations of Weyl and minimal super-energy observers in black hole spacetimes

机译:黑洞时空中Weyl和最小超能观测器的类电磁增强变换

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摘要

The transformation laws for the electric and magnetic parts of the electromagnetic 2-form and the Weyl tensor under a boost are studied using the complex vector approach, which shows the close analogy between the two cases. For a nonnull electromagnetic field, one can always find an observer who sees parallel electric and magnetic fields (vanishing Poynting vector) and also sees a minimum electromagnetic energy density (and minimum electric and magnetic field magnitudes) compared to other observers. For Weyl fields of all Petrov types except III, and boosts along certain directions of the Weyl principal tetrad, the more complicated Weyl transformation closely mimics the electromagnetic boost transformation, allowing one to : extend the electromagnetic results directly to the families of boosts along those directions. In particular for black hole spacetimes, the alignment of the electric and magnetic parts of the Weyl tensor (vanishing super-Poynting vector) leads to minimal gravitational super-energy as seen by the Carter observer within the family of all circularly rotating observers at each spacetime point outside the horizon. [References: 21]
机译:使用复矢量方法研究了升压下电磁2型和Weyl张量的电和磁部分的变换定律,表明了这两种情况之间的相似性。对于非零电磁场,总是可以找到一个观察者,与其他观察者相比,该观察者看到平行的电场和磁场(消失的Poynting矢量),并且看到最小的电磁能量密度(以及最小的电场和磁场强度)。对于除III以外的所有Petrov类型的Weyl场,并沿着Weyl主四面体的某些方向进行增强,更为复杂的Weyl变换紧密地模仿了电磁增强变换,从而可以:将电磁结果直接扩展到沿这些方向的增强族。特别是对于黑洞时空,Weyl张量的电气和磁性部分(消失的超珀因廷矢量)的对齐导致最小的引力超能,如卡特观测器在每个时空的所有循环旋转观测器族中所看到的那样指向地平线之外。 [参考:21]

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