Mendeley出力
＜図書＞
Supernovae and nucleosynthesis : an investigation of the history of matter, from the big bang to the present
| 責任表示 | David Arnett |
|---|---|
| シリーズ | Princeton series in astrophysics |
| データ種別 | 図書 |
| 出版者 | Princeton, N.J. : Princeton University Press |
| 出版年 | c1996 |
| 本文言語 | 英語 |
| 大きさ | xviii, 598 p. : ill. ; 24 cm |
| 概要 | This book investigates the question of how matter has evolved since its origin in the Big Bang, from the cosmological synthesis of hydrogen and helium to the generation of the complex set of nuclei th...t comprise our world and our selves. A central theme is the evolution of gravitationally contained thermonuclear reactors, otherwise known as stars. Our current understanding is presented systematically and quantitatively, by combining simple analytic models with new state-of-the-art computer simulations. The narrative begins with the clues (primarily the solar system abundance pattern), the constraining physics (primarily nuclear and particle physics), and the thermonuclear burning in the Big Bang itself. It continues with a step-by-step description of how stars evolve by nuclear reactions, a critical investigation of supernova explosion mechanisms and the formation of neutron stars and of black holes, and an analysis of how such explosions appear to astronomers (illustrated by comparison with recent observations). It concludes with a synthesis of these ideas for galactic evolution, with implications for nucleosynthesis in the first generation of stars and for the solar system abundance pattern. Emphasis is given to questions that remain open, and to active research areas that bridge the disciplines of astronomy, cosmochemistry, physics, and planetary and space science. Extensive references are given. This book investigates the question of how matter has evolved since its origin in the Big Bang, from the cosmological synthesis of hydrogen and helium to the generation of the complex set of nuclei that comprise our world and our selves. A central theme is the evolution of gravitationally contained thermonuclear reactors, otherwise known as stars. Our current understanding is presented systematically and quantitatively, by combining simple analytic models with new state-of-the-art computer simulations. The narrative begins with the clues (primarily the solar system abundance pattern), the constraining physics (primarily nuclear and particle physics), and the thermonuclear burning in the Big Bang itself. It continues with a step-by-step description of how stars evolve by nuclear reactions, a critical investigation of supernova explosion mechanisms and the formation of neutron stars and of black holes, and an analysis of how such explosions appear to astronomers (illustrated by comparison with recent observations). It concludes with a synthesis of these ideas for galactic evolution, with implications for nucleosynthesis in the first generation of stars and for the solar system abundance pattern. Emphasis is given to questions that remain open, and to active research areas that bridge the disciplines of astronomy, cosmochemistry, physics, and planetary and space science. Extensive references are given. 続きを見る |
所蔵情報
| 状態 | 巻次 | 所蔵場所 | 請求記号 | 刷年 | 文庫名称 | 資料番号 | コメント | 予約・取寄 | 複写申込 | 自動書庫 |
|---|---|---|---|---|---|---|---|---|---|---|
| : pbk | 理系図1F 開架 | 440.12/A 79/54960458 | 1996 |
|
054211996004582 |
|
||||
| : pbk | 【故障中】理系図 自動書庫 | 440.12/A 79/54960547 | 1996 |
|
054211996005471 |
|
書誌詳細
| 一般注記 | Includes bibliographical references (p. [573]-594) and index |
|---|---|
| 著者標目 | *Arnett, W. David (William David), 1940- |
| 件 名 | LCSH:Cosmology LCSH:Stars -- Evolution 全ての件名で検索 LCSH:Supernovae LCSH:Nucleosynthesis LCSH:Nucear astrophysics |
| 分 類 | LCC:QB981 DC20:523.1 NDC8:440.12 |
| 書誌ID | 1000007845 |
| ISBN | 0691011486 |
| NCID | BA27794350 |
| 巻冊次 | : alk. paper ; ISBN:0691011486 : pbk ; ISBN:0691011478 |
| 登録日 | 1997.01.27 |
| 更新日 | 1997.04.16 |