Non-Radial Pulsation of a Boson Star. I : Formulation : Astrophysics and Relativity
スポンサーリンク
概要
- 論文の詳細を見る
We shall investigate the non-radial pulsation of a boson star and the associated graviational waves. As the first step we here formulate the linearized perturbation around an equilibrium boson star in general relativity using the tensor harmonics and derive the perturbation equations for odd and even parity modes. It is found that the perturbations with odd parity do not couple with gravitational waves and the set of equations for even parity perturbations reduces to sixth-order system of differential equations.
- 理論物理学刊行会の論文
- 1991-08-25
著者
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FUTAMASE Toshifumi
Department of Astronomy, Graduate School of Science, Tohoku University
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Futamase Toshifumi
Department Of Physics Hirosaki University
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Futamase Toshifumi
Department Of Aeronautical Engineering Faculty Of Engineering Kyoto University
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Futamase Toshifumi
Astronomical Institute Graduate School Of Science Tohoku University
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Kojima Yasuaki
Graduate School Of Engineering Hiroshima University
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KOJIMA Yasufumi
Department of Physics, Tokyo Metropolitan University
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YOSHIDA Shijun
Department of Physics, Hirosaki University
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Yoshida Shijun
Department Of Physics Hirosaki University
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Kojima Y
Department Of Physics Hiroshima University
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Kojima Yasufumi
Department Of Physics Hiroshima University
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Kojima Yasufumi
Department Of Physics Tokyo Metropolitan University
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YOSHIDA Shijun
Astronomical Institute, Tohoku University
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KOJIMA Yasufumi
Department of Physics, Hiroshima University
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KOJIMA Yasufumi
Department of Physics, University of Wales
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Yosida Shijun
Department of Physics, Hirosaki University
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