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Published in 2022 at "Physical Review D"
DOI: 10.1103/physrevd.107.084031
Abstract: We calculate the spectrum of quasinormal modes of slowly rotating Kerr-Newman black holes. Using a perturbative double expansion method, second order in rotation and first order in non-radial perturbations, we obtain the system of equations…
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Keywords:
quasinormal modes;
kerr newman;
rotating kerr;
newman black ... See more keywords