The r-process element abundance with a realistic fission fragment mass distribution

S. Chiba, H. Koura, T. Maruyama, M. Ohta, S. Tatsuda, T. Wada, T. Tachibana, K. Sumiyoshi, K. Otsuki, T. Kajino

研究成果: Conference contribution

9 被引用数 (Scopus)

抄録

Effect of the β-delayed fission in r-process abundance is investigated with a realistic model for the fission fragment mass distribution (FFMD). The data base for the FFMD is constructed based on the two-center shell model and multi-dimensional Langevin calculation. The β-decay rates including neutron emission and β-delayed fission are also newly calculated with 2nd version of the the gross theory. The differences appeared in the final element abundance calculated with and without fission process, with different β-delayed fission rates are demonstrated.

本文言語English
ホスト出版物のタイトルOrigin of Matter and Evolution of Galaxies - 10th International Symposium on Origin of Matter and Evolution of Galaxies
ホスト出版物のサブタイトルFrom the Dawn of Universe to the Formation of Solar System, OMEG 2007
編集者Toshitaka Kajino, Takuma Suda, Takaya Nozawa, Akira Ohnishi, Masayuki Y. Fujimoto, Shigeru Kubono, Kiyoshi Kato
出版社American Institute of Physics Inc.
ページ162-167
ページ数6
ISBN(電子版)9780735405370
DOI
出版ステータスPublished - 2008
イベント10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, OMEG 2007 - Sapporo, Japan
継続期間: 2007 12月 42007 12月 7

出版物シリーズ

名前AIP Conference Proceedings
1016
ISSN(印刷版)0094-243X
ISSN(電子版)1551-7616

Other

Other10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, OMEG 2007
国/地域Japan
CitySapporo
Period07/12/407/12/7

ASJC Scopus subject areas

  • 物理学および天文学(全般)

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