Axial Gravitational Perturbations of Slowly-Rotating Compact Objects in General Relativity and Beyond
arXiv:2404.16437 · doi:10.1103/PhysRevD.110.064078
Abstract
We study the axial gravitational perturbations of slowly-rotating compact objects which are assumed to be supported by anisotropic fluids. We find that the gravitational perturbations decouple from the matter perturbations for axial sectors. We obtain a master wave equation whose potential is fully determined by the metric functions. This equation makes the calculations of gravitational QNMs for rotating compact objects extremely easy in specific background configurations.
latex, 14 pages, 1 figure; published version
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