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Parametrization of woods-saxon potential for heavy-ion systems 被引量:2
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作者 Lin Gan ZhiHong Li +18 位作者 HuiBin Sun DanYang Pang Bing Guo YunJu Li Jun Su ShengQuan Yan ErTao Li YouBao Wang Gang Lian ZhiYu Han XinYue Li DongHui Li tianli ma ChangJin Pei YangPing Shen Yi Su Sheng Zeng Yong Zhou WeiPing Liu 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2017年第8期28-34,共7页
Several elastic scattering angular distributions of ^(12)C from target nuclei of A ≥39 are analyzed to extract the Woods-Saxon potential parameters with the fixed imaginary potential and Coulomb radius parameters.Usi... Several elastic scattering angular distributions of ^(12)C from target nuclei of A ≥39 are analyzed to extract the Woods-Saxon potential parameters with the fixed imaginary potential and Coulomb radius parameters.Using the best fitted diffuseness parameters,the correlations of the real part parameters with A_1^(1/3)+ A_2^(1/3) and incident energy are revealed, and the systematic Woods-Saxon potential parameters are presented for nucleus-nucleus interaction.The proposed potential parameters can reproduce not only the elastic scattering angular distributions induced by ^(12)C,but also many elastic scattering angular distributions induced by the projectiles other than ^(12)C,thus providing important inputs for the study of nuclear reactions of heavy-ion systems. 展开更多
关键词 参数化 离子体 散射角分布 空间参数 扩散参数 最佳拟合 入射能量 相互作用
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New determination of astrophysical14C(n, γ)15C reaction rate from the spectroscopic factor of 15C 被引量:2
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作者 tianli ma Bing Guo +12 位作者 Dan Yang Pang ZhiHong Li Yi Su XinYue Li YangPing Shen YouBao Wang Yun Ju Li Jun Su ShengQuan Yan Sheng Zeng Gang Lian Ding Nan WeiPing Liu 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2020年第1期118-121,共4页
The14C(n,γ)15C reaction plays an important role in various astrophysical scenarios:(1)it is the slowest in the neutron induced CNO cycle which occurs in asymptotic giant branch(AGB)stars,and therefore controls this c... The14C(n,γ)15C reaction plays an important role in various astrophysical scenarios:(1)it is the slowest in the neutron induced CNO cycle which occurs in asymptotic giant branch(AGB)stars,and therefore controls this cycle[1];(2)it is one of the key reactions for predicting the primordial abundances of the heavy elements in the framework of inhomogeneous big-bang nucleosynthesis(IBBN)[2];(3)it is also important for the synthesis of heavier isotopes in neutrino driven wind scenarios for the r-process in core-collapse supernova(i.e.,Type-II supernova)explosions[3-5]. 展开更多
关键词 SPECTROSCOPIC CYCLE ASYMPTOTIC
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