A multispinor formalism is developed to derive the Teukolsky equation and compute quasi-normal modes for gravitational perturbations of six-dimensional rotating Kerr black holes, generalizable to other dimensions greater than four.
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Quasi-normal modes of a multi-dimensional rotating Kerr black hole
A multispinor formalism is developed to derive the Teukolsky equation and compute quasi-normal modes for gravitational perturbations of six-dimensional rotating Kerr black holes, generalizable to other dimensions greater than four.