Chapter 4 The Rotational Effects of General Relativity on the Stellar Pulsations
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概要
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Non-radial oscillations in slowly rotating stars are studied in the framework of general relativity. Slow rotation approximation is used, and the first order rotation effects on the perturbations are discussed from various aspects. The coupling of the modes, shift of the normal frequencies and quasi-toroidal oscillations are extensively reviewed here.
- 理論物理学刊行会の論文
- 1997-12-26
著者
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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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Kojima Y
Department Of Physics Hiroshima University
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Kojima Yasufumi
Department Of Physics Hiroshima University
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Kashiv Y.
Advanced Science Research Center Japan Atomic Energy Agency
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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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