Discrimination of Quark Stars from Neutron Stars in Quadrupole Oscillations
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概要
- 論文の詳細を見る
Frequencies and damping times due to gravitational radiation are calculated for self-bound quark star models. The results are compared with those for neutron star models, and it is found that they differ markedly in less relativistic cases. The difference derived here even based on a simple model of quark stars may be relevant to future theoretical and observational studies, because the oscillation properties depend essentially on the mass and radius for an equilibrium star.
- 理論物理学刊行会の論文
- 2002-11-25
著者
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SAKATA Koh-ichi
Department of Radiology, Sapporo Medical Univ.
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Kojima Yasuaki
Graduate School Of Engineering Hiroshima University
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Sakata Koh-ichi
Department Of Radiology Sapporo Medical University School Of Medicine
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Sakata Koh-ichi
Department Of Physics 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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SAKATA Koh-ichi
Department of Physics, Hiroshima University
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KOJIMA Yasufumi
Department of Physics, University of Wales
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