Challenge on the astrophysical r-process calculation with nuclear mass models
Meng Jie; Sun Bao-Hua; Sun, BH , Peking Univ, Sch Phys, Beijing 100871, Peoples R China
刊名CHINESE PHYSICS LETTERS
2008
卷号25期号:7页码:2429-2431
关键词Ground-state Properties Deformations Formula Stars
ISSN号0256-307X
英文摘要Our understanding of the rapid neutron capture nucleosynthesis process in universe depends on the reliability of nuclear mass predictions. Initiated by the newly developed mass table in the relativistic mean field theory (RMF), we investigate the influence of mass models on the r-process calculations, assuming the same astrophysical conditions. The different model predictions on the so far unreachable nuclei lead to significant deviations in the calculated r-process abundances.
学科主题Physics
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WOS记录号WOS:000257326000027
公开日期2012-08-02
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/5512]  
专题理论物理研究所_理论物理所1978-2010年知识产出
通讯作者Sun, BH , Peking Univ, Sch Phys, Beijing 100871, Peoples R China
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GB/T 7714
Meng Jie,Sun Bao-Hua,Sun, BH , Peking Univ, Sch Phys, Beijing 100871, Peoples R China. Challenge on the astrophysical r-process calculation with nuclear mass models[J]. CHINESE PHYSICS LETTERS,2008,25(7):2429-2431.
APA Meng Jie,Sun Bao-Hua,&Sun, BH , Peking Univ, Sch Phys, Beijing 100871, Peoples R China.(2008).Challenge on the astrophysical r-process calculation with nuclear mass models.CHINESE PHYSICS LETTERS,25(7),2429-2431.
MLA Meng Jie,et al."Challenge on the astrophysical r-process calculation with nuclear mass models".CHINESE PHYSICS LETTERS 25.7(2008):2429-2431.
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