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arXiv 2408.06985nucl-th
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裂变碎片退激过程中光学模型的不确定性量化

Uncertainty quantification of optical models in fission fragment de-excitation

Kyle A. Beyer, Amy E. Lovell, Cole D. Pruitt, Nathan P. Giha, Brian C. Kiedrowski

AI总结:

本研究通过蒙特卡罗 Hauser-Feshbach 形式传播两种光学势的不确定性至裂变观测量,发现中子能量相关观测量受光学模型不确定性影响显著,而某些实验特征需进一步研究。

摘要:

我们迈出了将天体物理相关能量下的复合核观测量纳入用于约束光学模型的实验证据的第一步,通过使用蒙特卡罗 Hauser-Feshbach 形式,将两个全局光学势(一个唯象的,一个微观的)的不确定性传播到相关的裂变观测量。我们将结果与广泛的历史和近期实验裂变测量进行比较,并详细讨论了不一致的区域。我们发现,在涉及中子能量的中子-碎片相关观测量中,参数化光学模型的不确定性是显著的。另一方面,我们观察到其他实验特征,特别是接近 $^{132}$Sn 壳层闭合处的中子-碎片相关性以及中子谱的高能分量,不太可能由光学势解释,需要进一步的实验和理论努力来解释。

英文摘要:

We take the first step towards incorporating compound nuclear observables at astrophysically relevant energies into the experimental evidence used to constrain optical models, by propagating the uncertainty in two global optical potentials, one phenomenological and one microscopic, to correlated fission observables using the Monte Carlo Hauser-Feshbach formalism. We compare to a wide range of historic and recent experimental fission measurements, and discuss in detail regions of disagreement. We find that the parametric optical model uncertainty in neutron-fragment correlated observables involving neutron energy is significant. On the other hand, we observe that other experimental features, particularly neutron-fragment correlations near the $^{132}$Sn shell-closure and the high energy component of neutron spectra, are unlikely to be explained by the optical potential, and will require further experimental and theoretical effort to explain.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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