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在新星环境下^(33)S(P,γ)^(34)Cl的热核反应率
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作者 隆建宏 张洁 罗志全 《西华师范大学学报(自然科学版)》 2011年第1期23-26,共4页
基于新测出的34Cl核共振能级的核物理信息,本文分析了在新星环境下33S(P,γ)34Cl的热核反应.本工作中同时考虑了非共振、共振两翼和窄共振对热核反应率的贡献,新星环境下33S(P,γ)34Cl的热核反应率的较统计模型给出的结果明显减少,最多... 基于新测出的34Cl核共振能级的核物理信息,本文分析了在新星环境下33S(P,γ)34Cl的热核反应.本工作中同时考虑了非共振、共振两翼和窄共振对热核反应率的贡献,新星环境下33S(P,γ)34Cl的热核反应率的较统计模型给出的结果明显减少,最多可下降约25%.结果可能影响到对新星抛射物中S同位素比率的预测(例如32S/33S),而这个比率可能会被用作新星前身星的一个诊断工具. 展开更多
关键词 非共振 共振 宽共振 热核反应率
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Proton capture reaction of ^(33)S in nova V1065 Centauri
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作者 罗志全 张洁 隆建宏 《Chinese Physics B》 SCIE EI CAS CSCD 2012年第9期613-616,共4页
Previous studies have shown that 33S(p,γ)34Cl is the most important reaction that affects the abundance of 33S in the product of nova nucleosynthesis. In this paper, a more accurate thermonuclear reaction rate of ... Previous studies have shown that 33S(p,γ)34Cl is the most important reaction that affects the abundance of 33S in the product of nova nucleosynthesis. In this paper, a more accurate thermonuclear reaction rate of 33S(p, γ)34Cl in the nova is calculated based on the newly measured 34C1 nuclear resonance levels. The electron screening correction and the non-resonance and narrow-resonance contributions are considered. The calculations are also combined with the recent observational data of nova V1065 Centauri and show that the thermonuclear reaction rates of 33S(p, γ) 34C1 are significantly different in the improved method. Because these results can affect the isotopic ratio of sulfur in the nova ejecta significantly, we make an estimate of the values of 328/33S and 338/338Q, which can be used as a diagnostic tool for the novae. 展开更多
关键词 NOVA NUCLEOSYNTHESIS METEORITE
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