Quasi-normal modes of Schwarzschild-de Sitter black holes

preprint2020arXivOpen access

Abstract

The low-laying frequencies of characteristic quasi-normal modes (QNM) of Schwarzschild-de Sitter (SdS) black holes have been calculated for fields of different spin using the 6th-order WKB approximation and the approximation by the Pöshl-Teller potential. The well-known asymptotic formula for large ll is generalized here on a case of the Schwarzchild-de Sitter black hole. In the limit of the near extreme ΛΛ term the results given by both methods are in a very good agreement, and in this limit fields of different spin decay with the same rate.

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