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Indirect Measurement of Astrophysical 13^C(a, n)^16O S-Factors
  • ISSN号:1009-0630
  • 期刊名称:《等离子体科学与技术:英文版》
  • 时间:0
  • 分类:O571.4[理学—粒子物理与原子核物理;理学—物理] P14[天文地球—天体物理;天文地球—天文学]
  • 作者机构:[1]China Institute of Atomic Energy, Beijing 102413, China, [2]School of Physics and State Key Laboratory of Nuclear Physics and Technology,Peking University, Beiiing 100871, China
  • 相关基金:supported by National Basic Research Program of China (No. 2007CB815003), National Natural Science Foundation of China(Nos. 10705053, 11021504, 10720101076, 10735100 and 10975193)
中文摘要:

The 13C(α,n)16O reaction is believed to be the main neutron source reaction for the s-process in asymptotic giant branch (AGB) stars. The astrophysical S-factors of this reaction have been determined based on an evaluation of the α spectroscopic factor of the 1/2+ subthreshold state in 17O (Ex=6.356 MeV) by using the 13C(11B,7Li)17O α transfer reaction. Our result confirms that the 1/2+ subthreshold resonance is dominant for the 13C(α,n)16O reaction at low energies of astrophysical interest.

英文摘要:

The 13^C(a, n)160 reaction is believed to be the main neutron source reaction for the s-process in asymptotic giant branch (AGB) stars. The astrophysical S-factors of this reaction have been determined based on an evaluation of the a spectroscopic factor of the 1/2+ subthreshold state in 17^O (Ex = 6.356 MeV) by using the 13^C(11^B, 7^Li)17^O a transfer reaction. Our result confirms that the 1/2+ subthreshold resonance is dominant for the 13^C(a, n)16^O reaction at low energies of astrophysical interest.

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期刊信息
  • 《等离子体科学与技术:英文版》
  • 主管单位:中国科学院 中国科协
  • 主办单位:中国科学院等离子体物理研究所 中国力学学会
  • 主编:万元熙、谢纪康
  • 地址:合肥市1126信箱
  • 邮编:230031
  • 邮箱:pst@ipp.ac.cn
  • 电话:0551-5591617 5591388
  • 国际标准刊号:ISSN:1009-0630
  • 国内统一刊号:ISSN:34-1187/TL
  • 邮发代号:
  • 获奖情况:
  • 国内外数据库收录:
  • 美国化学文摘(网络版),荷兰文摘与引文数据库,美国工程索引,美国剑桥科学文摘,美国科学引文索引(扩展库),英国科学文摘数据库
  • 被引量:89