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The objective of this paper is to construct the accurate (say, to 11 decimal places) frequencies of the quasinormal modes of the 5-dimensional Schwarzschild-Tangherlini black hole using three major techniques: the Hill determinant method, the continued fractions method and the WKB-Pad\'e method and to discuss the limitations of each.
P. P. Fiziev (2019), eprint arXiv:1912.13432
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