Constraining Nuclear-Matter Equations of State by Gravitational Waves from Black Hole-Neutron Star Binaries(Nuclear Astrophysics,New Frontiers in QCD 2010-Exotic Hadron Systems and Dense Matter-)
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概要
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The waveform of gravitational waves from the final stage of coalescing low-mass black hole-neutron star binaries depends sensitively on the equation of state of neutron star matter. We show that the observation of such gravitational waves can lead to constraining the nuclear-matter equations of state.
- 理論物理学刊行会の論文
- 2010-12-17
著者
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Shibata Masaru
Yukawa Institute For Theoretical Physics Kyoto University
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KYUTOKU Koutarou
Yukawa Institute for Theoretical Physics, Kyoto University
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Kyutoku Koutarou
Yukawa Institute For Theoretical Physics Kyoto University
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SHIBATA Masaru
Yukawa Institute for Theoretical Physics, Kyoto University
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