Dynamical instability of ultra-spinning myers-perry black holes

Keiju Murata, Norihiro Tanahashi, Takahiro Tanaka

Research output: Contribution to conferencePaper

Abstract

We study the dynamical stability of Myers-Perry black holes with single rotation parameter. We derived the gravitational perturbation equation of the most symmetric mode, which is given by a system of partial differential equations. We solve the partial differential equations by the relaxation method and find the marginally stable modes in d = 6, 7 dimensions. This result indicates not only the instability of Myers-Perry black holes with a large angular momentum, but also the existence of a sequence of new black hole solutions in d ≥ 6 dimensions.

Original languageEnglish
Pages243-246
Number of pages4
Publication statusPublished - 2009 Dec 1
Event19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009 - Tokyo, Japan
Duration: 2009 Nov 302009 Dec 4

Other

Other19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009
CountryJapan
CityTokyo
Period09/11/3009/12/4

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ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

Cite this

Murata, K., Tanahashi, N., & Tanaka, T. (2009). Dynamical instability of ultra-spinning myers-perry black holes. 243-246. Paper presented at 19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009, Tokyo, Japan.