2010年
Constraining Nuclear-Matter Equations of State by Gravitational Waves from Black Hole-Neutron Star Binaries
Progress of Theoretical Physics Supplement
- ,
- 巻
- 186
- 号
- 186
- 開始ページ
- 17
- 終了ページ
- 25
- 記述言語
- 英語
- 掲載種別
- 研究論文（学術雑誌）
- DOI
- 10.1143/PTPS.186.17
- 出版者・発行元
- PROGRESS THEORETICAL PHYSICS PUBLICATION OFFICE
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.
- リンク情報
- ID情報
-
- DOI : 10.1143/PTPS.186.17
- ISSN : 0375-9687
- ORCIDのPut Code : 51254129
- Web of Science ID : WOS:000285731300004