Quasi-normal modes of Schwarzschild-de Sitter black holes

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 P\"oshl-Teller potential. The well-known asymptotic formula for large l is generalized here on a case of the Schwarzchild-de Sitter black hole. In the limit of the near extreme 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.

0

Turn this paper into a full lesson

ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.

Discussion (0)

Sign in to join the discussion.

Loading comments…