2007年8月
Modeling dense stellar systems
PROGRESS OF THEORETICAL PHYSICS
- ,
- ,
- ,
- 巻
- 118
- 号
- 2
- 開始ページ
- 187
- 終了ページ
- 209
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1143/PTP.118.187
- 出版者・発行元
- PROGRESS THEORETICAL PHYSICS PUBLICATION OFFICE
Black holes and neutron stars present extreme forms of matter that cannot be created as such in a laboratory on Earth. Instead, we have to observe and analyze the experiments that are ongoing in the Universe. The most telling observations of black holes and neutron stars come from dense stellar systems, where stars are crowded close enough to each other to undergo frequent interactions. It is the interplay between black holes, neutron stars and other objects in a dense environment that allows us to use observations to draw firm conclusions about the properties of these extreme forms of matter, through comparisons with simulations. The art of modeling dense stellar systems through computer simulations forms the main topic of this review.
- リンク情報
- ID情報
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- DOI : 10.1143/PTP.118.187
- ISSN : 0033-068X
- CiNii Articles ID : 110006379786
- Web of Science ID : WOS:000249333700001