R-process nucleosynthesis in supernova explosion

M. Saruwatari, Masa-Aki Hashimoto, K. Kotake, S. Yamada

研究成果: Chapter in Book/Report/Conference proceedingConference contribution

抜粋

We investigate the possibility of the r-process during the magnetohydrodynamical (MHD) explosion of supernova in a massive star of 13M with the effects of neutrinos included. Contrary to the case of the spherical explosion, jet-like explosion due to the combined effects of rotation and magnetic field lowers the electron fraction significantly inside the layers. We find that the ejected material of low electron fraction responsible for the r-process comes out from the inner deep region of the core that is made up of iron-group nuclei. This leads to the production of the second to third peak in the solar r-process elements. We suggest that there are some variations in the r-process nucleosynthesis according to the initial conditions of rotational and magnetic fields.

元の言語英語
ホスト出版物のタイトルFrontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3
ページ420-422
ページ数3
DOI
出版物ステータス出版済み - 11 24 2011
イベント3rd International Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3 - Rhodes, ギリシャ
継続期間: 8 23 20108 27 2010

出版物シリーズ

名前AIP Conference Proceedings
1377
ISSN(印刷物)0094-243X
ISSN(電子版)1551-7616

その他

その他3rd International Conference on Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3
ギリシャ
Rhodes
期間8/23/108/27/10

All Science Journal Classification (ASJC) codes

  • Ecology, Evolution, Behavior and Systematics
  • Ecology
  • Plant Science
  • Physics and Astronomy(all)
  • Nature and Landscape Conservation

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  • これを引用

    Saruwatari, M., Hashimoto, M-A., Kotake, K., & Yamada, S. (2011). R-process nucleosynthesis in supernova explosion. : Frontiers in Nuclear Structure, Astrophysics, and Reactions, FINUSTAR 3 (pp. 420-422). (AIP Conference Proceedings; 巻数 1377). https://doi.org/10.1063/1.3628432