Scalar quasinormal modes of Kerr-AdS(5)

Julian Barragan Amado*, Bruno Carneiro da Cunha, Elisabetta Pallante

*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

27 Citations (Scopus)
184 Downloads (Pure)

Abstract

An analytic expression for the scalar quasinormal modes of generic, spinning Kerr-AdS(5) black holes was previously proposed by the authors [J. High Energy Phys. 08 (2017) 094], in terms of transcendental equations involving the Painlev'e VI (PVI) tau function. In this work, we carry out a numerical investigation of the modes for generic rotation parameters, comparing implementations of expansions for the PVI tau function in terms of both conformal blocks (Nekrasov functions) and Fredholm determinants. We compare the results with standard numerical methods for the subcase of Schwarzschild black holes. We then derive asymptotic formulas for the angular eigenvalues and the quasinormal modes in the small black hole limit for generic scalar mass and discuss, both numerically and analytically, the appearance of superradiant modes.

Original languageEnglish
Article number105006
Number of pages21
JournalPhysical Review D
Volume99
Issue number10
DOIs
Publication statusPublished - 15-May-2019

Keywords

  • EQUATIONS

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