Improving nuclear data evaluations with predictive reaction theory and indirect measurements

J. Escher, Kirana Bergstrom, E. Chimanski, O. Gorton, E. J. In, M. Kruse, S. P'eru, C. Pruitt, R. Rahman, Emily Shinkle, Aaina Thapa, W. Younes
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Abstract

Nuclear reaction data required for astrophysics and applications is incomplete, as not all nuclear reactions can be measured or reliably predicted. Neutron-induced reactions involving unstable targets are particularly challenging, but often critical for simulations. In response to this need, indirect approaches, such as the surrogate reaction method, have been developed. Nuclear theory is key to extract reliable cross sections from such indirect measurements. We describe ongoing efforts to expand the theoretical capabilities that enable surrogate reaction measurements. We focus on microscopic predictions for charged-particle inelastic scattering, uncertainty-quantified optical nucleon-nucleus models, and neural-network enhanced parameter inference.
用预测反应理论和间接测量改进核数据评价
天体物理学和应用所需的核反应数据是不完整的,因为并非所有的核反应都可以测量或可靠地预测。涉及不稳定目标的中子诱导反应尤其具有挑战性,但通常对模拟至关重要。为了满足这一需求,人们开发了间接方法,如替代反应法。核理论是从这种间接测量中提取可靠截面的关键。我们描述了正在进行的努力,以扩大理论能力,使替代反应测量。我们专注于带电粒子非弹性散射的微观预测,不确定性量化光学核子-核子模型,以及神经网络增强的参数推理。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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