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We calculate the scalar-gravitational quasi-normal modes of equal angular momenta Myers-Perry black holes in odd dimensions.
New York, NY: Gordon and Breach, 1973
B. Carter, Black Hole Equilibrium States II: General Theory of Stationary Black Hole States · 1973
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S. A. Teukolsky, Perturbations of a rotating black hole. 1. Fundamental equations for gravitational electromagnetic and neutrino field perturbations
1973
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1986
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R. Emparan and R. C. Myers, Instability of ultra-spinning black holes
2003
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H. Kodama and A. Ishibashi, A Master equation for gravitational perturbations of maximally symmetric black holes in higher dimensions
2003
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V. Cardoso and O. J. Dias, Small Kerr-anti-de Sitter black holes are unstable
2004
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H. K. Kunduri, J. Lucietti, and H. S. Reall, Gravitational perturbations of higher dimensional rotating black holes: Tensor perturbations
2006
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O. J. Dias, R. Monteiro, and J. E. Santos, Ultraspinning instability: the missing link
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2009
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E. Berti, V. Cardoso, and A. O. Starinets, Quasinormal modes of black holes and black branes
2009
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R. Emparan, T. Harmark, V. Niarchos, and N. A. Obers, New Horizons for Black Holes and Branes
2010
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2011
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Cambridge University Press, 2012
G. T. Horowitz, ”Black Holes in Higher Dimensions” · 2012
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R. Emparan, R. Suzuki, and K. Tanabe, The large D limit of General Relativity
2013
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