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MEASUREMENT OF THE 330 keV RESONANCE IN ~(18)F(p,α)~(15)O

机译:〜(18)F(p,α)〜(15)O中330 keV共振的测量

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While recent measurements have substantially improved our understanding of the ~(18)F(p,α)~(15)O reaction that is important in novae, the production of ~(18)F is still uncertain by more than 2 orders of magnitude, due in large part to the contribution of a resonance located at E_(cm) = 330 keV. We developed a new technique to study resonant (p, α) reactions and employed it to measure properties of the E_(cm) = 183 keV resonance in ~(17)O(p, α)~(14)N which had been previously reported to decrease ~(18)F production in ONeMg novae by as much as a factor of 10. The previous results were confirmed using the new technique and we now propose to use this technique to study the ~(18)F(p, α)~(15)O reaction.
机译:尽管最近的测量已大大改善了我们对新星中重要的〜(18)F(p,α)〜(15)O反应的理解,但〜(18)F的产生仍不确定2个数量级以上,主要是由于位于E_(cm)= 330 keV处的共振的影响。我们开发了一种研究共振(p,α)反应的新技术,并将其用于测量先前已经存在的〜(17)O(p,α)〜(14)N中E_(cm)= 183 keV共振的性质据报道,它能使新的ONeMg新星中的〜(18)F产生降低多达10倍。以前的结果已使用新技术得到证实,我们现在建议使用该技术来研究〜(18)F(p,α )〜(15)O反应。

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