首页> 外文期刊>The Astrophysical journal >MEASUREMENT OF THE ~(16)O(n, γ)~(17)O REACTION CROSS SECTION AT STELLAR ENERGY AND THE CRITICAL ROLE OF NONRESONANT p-WAVE NEUTRON CAPTURE
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MEASUREMENT OF THE ~(16)O(n, γ)~(17)O REACTION CROSS SECTION AT STELLAR ENERGY AND THE CRITICAL ROLE OF NONRESONANT p-WAVE NEUTRON CAPTURE

机译:星能下〜(16)O(n,γ)〜(17)O反应截面的测量及非共振p波中子俘获的临界作用

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摘要

The cross section of the ~(16)O(n, γ)~(17)O reaction, important for nucleosynthesis theories of s and p processes and of inhomogeneous big bang models, has been measured at stellar neutron energy. The Maxwellian-averaged cross section at kT = 30 keV was derived as 34 ± 4 μbarn; 170 times larger than the value reported previously. The results could significantly alter the s and p process efficiencies in metal-deficient stars due to a strong neutron poison of ~(16)O and increase the primordial nucleosynthesis yield in inhomogeneous models. The large cross section is attributed to a nonresonant p-wave neutron-capture process. It is pointed out that this process plays an important role in the neutron-capture reaction of light nuclei at stellar energy; the cross section deviates considerably from the extrapolated value of the measured thermal-capture cross section by assuming a 1/v law and therefore the process significantly influences both the stellar and above-mentioned primordial nucleosynthesis theories.
机译:在恒星中子能量下测量了〜(16)O(n,γ)〜(17)O反应的横截面,这对于s和p过程的核合成理论以及非均质的大爆炸模型都很重要。在kT = 30 keV时的麦克斯韦平均截面为34±4μbarn。比以前报告的值大170倍。结果可能会由于〜(16)O的强中子毒害而显着改变缺金属恒星的s和p过程效率,并增加非均质模型中原始核合成的产率。大横截面归因于非共振p波中子捕获过程。指出这一过程在恒星能量下光核的中子捕获反应中起着重要作用。通过假设1 / v定律,横截面与测得的热捕获横截面的外推值有很大的出入,因此该过程显着影响了恒星和上述原始核合成理论。

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