Effects of a new 3-alpha reaction on the s-process in massive stars

Yukihiro Kikuch, Masaomi Ono, Yasuhide Matsuo, Masa-Aki Hashimoto, Shin Ichiro Fujimoto

研究成果: 書籍/レポート タイプへの寄稿会議への寄与

抄録

Effect of a new 3-alpha reaction rate on the s-process during the evolution of a massive star of 25 solar mass is investigated for the first time, because the s-process in massive stars have been believed to be established with only minor change. We find that the s-process with use of the new rate during the core helium burning is very inefficient compared to the case with the previous 3-alpha rate. However, the difference of the overproduction is found to be largely compensated by the subsequent carbon burning. Since the s-process in massive stars has been attributed so far to the neutron irradiation during core helium burning, our finding reveals for the first time the importance of the carbon burning for the s-process during the evolution of massive stars.

本文言語英語
ホスト出版物のタイトルOrigin of Matter and Evolution of Galaxies 2011
ページ384-386
ページ数3
DOI
出版ステータス出版済み - 12月 1 2012
イベントInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, 日本
継続期間: 11月 14 201111月 17 2011

出版物シリーズ

名前AIP Conference Proceedings
1484
ISSN(印刷版)0094-243X
ISSN(電子版)1551-7616

その他

その他International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
国/地域日本
CityWako
Period11/14/1111/17/11

!!!All Science Journal Classification (ASJC) codes

  • 生態、進化、行動および分類学
  • 生態学
  • 植物科学
  • 物理学および天文学(全般)
  • 自然保全および景観保全

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