Teichmuller Motion of (2+1)-Dimensional Gravity with the Cosmological Constant : Astrophysics and Relativity
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概要
- 論文の詳細を見る
The (2+1)-dimensional Einstein gravity with a cosmological constant is studied in the ADM canonical formalism. Adopting York's time slice, we completely solve the initial-value problem and the time evolution equations with an initial spacelike 2-surface being a closed Riemann surface of genus zero and one. The result in a torus case is that the Teichmuller parameters for the torus follow a geodesic in the Teichmuller space but its motion asymptotically stops due to the presence of the cosmological constant.
- 理論物理学刊行会の論文
- 1990-04-25
著者
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SODA Jiro
Department of Physics, Kyoto University
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SODA Jiro
Research Institute for Theoretical Physics Hiroshima University
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Soda Jiro
Reaearch Institute For Theoretical Physics Hiroshima University
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FUJIWARA Yoshihisa
Research Institute for Theoretical Physics, Hiroshima University
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FUJIWARA Yoshikazu
School of Physics, University of Minnesota
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FUJIWARA Yoshikazu
Research Institute for Fandamental Physics, Kyoto University
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Fujiwara Yoshihisa
Research Institute For Theoretical Physics Hiroshima University
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FUJIWARA Yoshikazu
Institute of Theoretical Physics, University of Regensburg : Department of Physics, Kyoto University
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