0.3A-1.5A GeV - 56Fe+p反应产生剥落残渣经验公式的验证

N. Nicolis, Theodora-Ilektra Katsigianni, Kostantinos Korakas, Athanasia Miliadou, Diamantis Tasioudis
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引用次数: 0

摘要

用宇宙射线天体物理学、活化研究和医学应用同位素生产中经常使用的经验参数公式描述了56Fe+p轰击中碎裂残余物的产生。将质量、电荷和同位素分布等实验观测值与Rudstam和Silberberg-Tsao两种公式和SPACS公式的计算结果进行了比较。并与两阶段反应模型的预测结果作了比较,以供参考。报道了这些方法得到的偏差系数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Validation of Empirical Formulas for Spallation Residue Production in 0.3A-1.5A GeV 56Fe+p Reactions
The production of spallation residues in 56Fe+p bombardments is described with empirical parametric formulas often used in cosmic-ray astrophysics, activation studies and isotope production for medical applications. Experimental observables including mass, charge and isotopic distributions are compared with calculations using two versions of the formulas of Rudstam and Silberberg-Tsao and the SPACS formula.  For reference, a comparison is made with the predictions of a two-stage reaction model. Deviation factors obtained in these approaches are reported.
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