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采用EMU01国际合作组的原子核乳胶为探测器，系统地研究了能量为14．6、60、200GeV／u的~(16)O核、200GeV／u的~(32)S核诱发核反应中产生的灰粒子平均多重数及角分布。以描写相对论性核-核碰撞的LUCIAE模型为基础，进行MonteCarlo模拟的结果与实验数据一致。
Using the nuclear emulsion of EMU01 International Cooperation Group as the detector, we have systematically studied the nuclear-induced nuclear reactions induced by ~ (16) O nuclei with energies of 14.6, 60,200 GeV / u and ~20 The average multiplicity and angular distribution of gray particles. Based on the LUCIAE model describing relativistic nuclear-nuclear collisions, the Monte Carlo simulations are consistent with the experimental data.