The decay of fission fragments is studied throughMonte Carlo Hauser-Feshbach model calculations taking into account the competition between the emissions of prompt fission neutrons and gamma rays. The importance of initial excitation energy and spin distribution in the primary light and heavy fragments is demonstrated through comparison with experimental data. Excitation energy sorting mechanisms at scission are discussed in the light of these advanced simulations. Preliminary results on prompt fission gamma rays are also reported.
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机译：通过Montee Carlo Hauser-Feshbach模型计算研究了裂变片段的衰减，考虑到迅速裂变中子和伽马射线的排放之间的竞争。通过与实验数据进行比较，证明了初始励磁能量和旋转分布在初级光和重碎片中的重要性。鉴于这些高级模拟讨论了侦察时的激发能量分类机制。报告了促进裂变伽马光线的初步结果。
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