Higher-Dimensional Numerical Relativity : Current Status(Chapter 9,Higher Dimensional Black Holes)
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概要
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We summarize the current status of numerical relativity for higher-dimensional spacetimes. In the first part, the ingredients necessary for successful simulations developed to date are summarized, including formulations, methods of implementing spacetime symmetries, and gauge conditions. In the second part, we review the simulations performed so far, such as time evolution of a black string that is unstable against the Gregory-Laflamme instability, black hole collisions and scatterings, and time evolution of rapidly rotating Myers-Perry (MP) black holes with one rotational parameter which are unstable against bar-mode deformation. The remaining issues and expected future developments are briefly described.
- 2011-08-29
著者
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Shibata Masaru
Yukawa Institute For Theoretical Physics Kyoto University
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Yoshino Hirotaka
Cosmophysics Group Institute Of Particles And Nuclear Studies Kek
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SHIBATA Masaru
Yukawa Institute for Theoretical Physics, Kyoto University
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YOSHINO Hirotaka
Cosmophysics Group, Institute of Particles and Nuclear Studies, KEK
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