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New determination of astrophysical14C(n, γ)15C reaction rate from the spectroscopic factor of 15C 被引量:2

New determination of astrophysical14C(n, γ)15C reaction rate from the spectroscopic factor of 15C
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摘要 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].
出处 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2020年第1期118-121,共4页 中国科学:物理学、力学、天文学(英文版)
基金 supported by the National Key Research and Development Project(Grant No.2016YFA0400502) the National Natural Science Foundation of China(Grant Nos.11490561,11475264,11475265,and11575292) the National Program on Key Basic Research Project of China(Grant No.2013CB834406)
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