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We use the continued fraction method to determine the eigenfrequencies associated with a scalar field around a Kerr-like black hole. The Kerr-like metric considered in this article is a subclass of the general parametrization of axisymmetric black ho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f81c8f3670a45864a41004db7fafcba1
