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Null geodesics, quasinormal modes of a massless scalar field perturbation and the correspondence with shadow radii are investigated in the background spacetime of high-dimensional Einstein-Yang-Mills black holes.
1903
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1904
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1906
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1909
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R.A. Konoplya, Quantum corrected black holes: Quasinormal modes, scattering, shadows
1912
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1912
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1912
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J.M. Bardeen, W.H. Press, and S. A. Teukolsky, Rotating black holes: Locally nonrotating frames, energy extraction, and scalar synchrotron radiation
1972
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S. Iyer and C. M. Will, Black-hole normal modes: A WKB approach. I. Foundations and application of a higher-order WKB analysis of potential-barrier scattering
1987
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R.M. Corless, G.H. Gonnet, D.E.G. Hare, D.J. Jeffrey, and D.E. Knuth, On the Lambert W function
1996
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L. Motl and A. Neitzke, An analytical computation of asymptotic Schwarzschild quasinormal frequencies
2003
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L. Motl and A. Neitzke, Asymptotic black hole quasinormal frequencies
2003
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2003
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L. Fidkowski, V. Hubeny, M. Kleban, and S. Shenker, The black hole singularity in AdS/CFT
2004
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K. Jusufi, Connection between the shadow radius and quasinormal modes in rotating spacetimes
2004
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2008
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2008
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A. Starinets, Quasinormal spectrum and the black hole membrane paradigm
2009
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2009
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S.E. Vazquez and E.P. Esteban, Strong field gravitational lensing by a Kerr black hole
2004
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2005
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Y. Guo and Y.-G. Miao, Scalar quasinormal modes of black holes in Einstein-Yang-Mills gravity
2005
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G. Festuccia and H. Liu, Excursions beyond the horizon: Black hole singularities in Yang-Mills theories
2006
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I. Sachs, Quasi-normal modes for logarithmic conformal field theory
2008
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2008
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2010
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2010
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2015
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2016
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2017
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J. Matyjasek and M. Opala, Quasinormal modes of black holes: The improved semianalytic approach
2017
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