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Impacts of the New Carbon Fusion Cross Sections on Type Ia Supernovae

  • Kanji Mori*
  • , Michael A. Famiano
  • , Toshitaka Kajino
  • , Motohiko Kusakabe
  • , Xiaodong Tang
  • *此作品的通讯作者
  • National Astronomical Observatory of Japan
  • The University of Tokyo
  • Beihang University
  • Western Michigan University
  • CAS - Institute of Modern Physics

科研成果: 书/报告/会议事项章节 › 会议稿件 › 同行评审

摘要

Recent measurement of cross sections of the carbon fusion reaction unveiled existence of low-energy resonances, which enhances reaction rates. We apply the new resonant reaction rates to the double degenerate scenario of type Ia supernovae. It is shown that merging carbon-oxygen white dwarfs are more likely to be burnt into oxygen-neon-magnesium white dwarfs by the enhanced reaction rates and collapse into neutron stars.

源语言英语
主期刊名Nuclei in the Cosmos XV
编辑Alba Formicola, Matthias Junker, Lucio Gialanella, Gianluca Imbriani
出版商Springer Science and Business Media, LLC
页409-412
页数4
ISBN(印刷版)9783030138752
DOI
出版状态已出版 - 2019
活动15th International Symposium on Nuclei in the Cosmos, NIC 2018 - L'Aquila, 意大利
期限: 24 6月 2018 → 29 6月 2018

丛书

姓名Springer Proceedings in Physics
卷219
ISSN(印刷版)0930-8989
ISSN(电子版)1867-4941

会议

会议15th International Symposium on Nuclei in the Cosmos, NIC 2018
国家/地区意大利
市L'Aquila
时期24/06/18 → 29/06/18

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