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Formation of the Bubbly Universe by Cumulative Explosions
https://ir.soken.ac.jp/records/4264
https://ir.soken.ac.jp/records/42649a7e1987-3eca-4c14-80f7-78f65004f64a
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2014-02-19 | |||||
| タイトル | ||||||
| タイトル | Formation of the Bubbly Universe by Cumulative Explosions | |||||
| タイトル | ||||||
| タイトル | Formation of the Bubbly Universe by Cumulative Explosions | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| 資源タイプ | ||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
| 資源タイプ | journal article | |||||
| 著者 |
YOSHIOKA, Satoshi
× YOSHIOKA, Satoshi× IKEUCHI, Satoru |
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| 著者別名 |
池内, 了
× 池内, 了 |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | The scale of structures of the universe which can be produced in the explosion scenario is investigated. Solving the equation of motion of an expanding shell produced by cosmic explosions based on the thin-shell approximation, it is shown that it is possible that bubbles of size about 40 Mpc are formed by successive explosions starting from the first-generation objects. However, the observed isotropy of the microwave background radiation limits the bubble size to less than about 30 Mpc in the simple explosion scenario. | |||||
| 書誌情報 |
Publications of the Astronomical Society of Japan en : Publications of the Astronomical Society of Japan 巻 40, 号 4, p. 383-401, 発行日 1988 |
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| 出版者 | ||||||
| 出版者 | The Astronomical Society of Japan | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 0004-6264 | |||||
| 権利 | ||||||
| 権利情報 | © The Astronomical Society of Japan | |||||
| 関連サイト | ||||||
| 識別子タイプ | URI | |||||
| 関連識別子 | http://pasj.asj.or.jp/info/subscription.html | |||||
| 関連名称 | Copyright | |||||
| フォーマット | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | application/pdf | |||||
| 著者版フラグ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
