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High-precision (p,t) Reactions to DetermineReaction Rates in the Stellar rp-process

机译:高精度(P,T)对恒星RP-Process的测定率的反应

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The main source of uncertainties in stellar rate calculations of the rp-process and the competing αp-process is often the lack of knowledge of the resonance states above the p- and α-thresholds and their precise energies. We have started a program to study these resonances in proton-rich unstable nuclei via the (p,t) and other neutron-pickup reactions using the high resolution spectrometer Grand Raiden. Here, we are presenting the status of the project and recent results of the ~(25)Al(p,γ) reaction rates based on the analysis of measured ~(28)Si(p,t)~(26)Si spectra.
机译:RP-Process和竞争αp过程的恒星速率计算中的不确定性的主要来源通常是对P - 和α-阈值和其精确能量的共振状态缺乏了解。我们已经开始通过使用高分辨率光谱仪Grand Raiden的(P,T)和其他中子拾取反应来研究质子 - 富有的不稳定核中的这些共振。在此,我们基于测量〜(28)Si(P,T)〜(26)Si光谱的分析,介绍〜(25)Al(P,γ)反应速率的〜(25)Al(P,γ)反应速率的最新结果。

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