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On Kerr black hole deformations admitting a Carter constant and an invariant criterion for the separability of the wave equation
General Relativity and Gravitation ( IF 2.8 ) Pub Date : 2021-02-22 , DOI: 10.1007/s10714-021-02795-2 Georgios O. Papadopoulos , Kostas D. Kokkotas
中文翻译:
关于Kerr黑洞变形,该变形允许Carter常数和波动方程可分离性的不变准则。
更新日期:2021-02-22
General Relativity and Gravitation ( IF 2.8 ) Pub Date : 2021-02-22 , DOI: 10.1007/s10714-021-02795-2 Georgios O. Papadopoulos , Kostas D. Kokkotas
In a previous work of ours, the most general family of Kerr deformations—admitting a Carter constant—has been presented. This time a simple, necessary and sufficient condition in order for the aforementioned family to have a separable Klein-Gordon equation is exhibited. In addition, we provide a solid theoretical foundation that the maximum number of free to be chosen radial functions is three.
中文翻译:
关于Kerr黑洞变形,该变形允许Carter常数和波动方程可分离性的不变准则。
在我们先前的工作中,提出了最普通的Kerr变形族(允许Carter常数)。这次展示了简单,必要和充分的条件,以使上述族具有可分离的Klein-Gordon方程。此外,我们提供了坚实的理论基础,即自由选择的径向函数的最大数量为3。