R-process nucleosynthesis during the magnetohydrodynamics explosions of a massive star

Motoaki Saruwatari*, Masa Aki Hashimoto, Kei Kotake, Shoichi Yamada

*この研究の対応する著者

研究成果: Conference contribution

抄録

We investigate the possibility of the r-process during the magnetohydrohynamical explosion of supernova in a massive star of 13 solar mass with the effects of neutrinos induced. We adopt five kinds of initial models which include properties of rotation and the toroidal component of the magnetic field. The simulations which succeed the explosions are limitted to a concentrated magnetic field and strong differential rotation. Low Ye ejecta produce heavy elements and the third peak can be reprocuced. However, the second peak is low because Ye distribution as a function of radius is steep and ejecta corresponding to middle Ye is very few.

本文言語English
ホスト出版物のタイトル10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10
ページ409-411
ページ数3
DOI
出版ステータスPublished - 2010 9月 21
イベント10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10 - Osaka, Japan
継続期間: 2010 3月 82010 3月 10

出版物シリーズ

名前AIP Conference Proceedings
1269
ISSN(印刷版)0094-243X
ISSN(電子版)1551-7616

Conference

Conference10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10
国/地域Japan
CityOsaka
Period10/3/810/3/10

ASJC Scopus subject areas

  • 物理学および天文学(全般)

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