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作 者:胡荣江[1] 肖志刚[1] 吴和宇[1] 段利敏[1] 王宏伟[1] 袁小华[1] 靳根明[1] 诸永泰[1] 李祖玉[1] 王素芳[1] 徐瑚珊[1] 张保国[1] 魏志勇[1] 冯兆庆[1] 付芬[1]
出 处:《高能物理与核物理》2007年第4期350-356,共7页High Energy Physics and Nuclear Physics
基 金:国家自然科学基金(10205020;19575055;10175081);国家重点基础研究发展规划项目(G2000077401);中国科学院知识创新工程方向性项目(KJCX2-SW-N18)资助~~
摘 要:测量了35MeV/u36Ar+112,124Sn反应中小角关联出射的中等质量碎片(IMF)约化速度关联函数.结果表明36Ar+124Sn反应系统中的约化速度关联函数在小约化速度处的反关联程度比36Ar+112Sn反应系统中的强,表现出明显的入射道依赖性.考察出射粒子对的单核子总动量时,发现这种差异主要来自于高动量粒子对的贡献.用三体弹道理论模型MENEKA分别计算了两个系统的IMF发射时标,在36Ar+112Sn反应系统中约为150fm/c,而在36Ar+124Sn反应系统中,约为120fm/c.同位旋相关的量子分子动力学计算表明,36Ar+124Sn系统中IMF的发射时间谱比36Ar+112Sn系统略有前移,相应地,其中心密度从最高点随时间的下降亦比36Ar+112Sn系统略快.The reduced velocity correlation functions of the Intermediate Mass Fragments (IMFs) were measured in the reactions of ^36Ar+^112,^124Sn at 35MeV/u. The anti-correlation at small reduced velocities is more pronounced in ^36Ar+^124Sn system than that in ^36Ar+^112Sn system. The difference of the correlation functions between the two reactions is mainly contributed by the particle pairs with high momenta. A three-body Coulomb repulsive trajectory code (MENEKA) is employed to calculate the emission time scale of IMFs for the both systems. The time scale is 150fm/c in the ^36Ar+^112Sn system and 120fm/c in the ^36Ar+^124Sn system, respectively. A calculation based on an Isospin dependence Quantum Molecular Dynamics code (IQMD) reveals that the emission time spectrum of IMFs is shifted slightly leftwards in ^36Ar+^124Sn compared with that in the ^36Ar+^112Sn system, indicating a shorter emission time scale. Correspondingly, the central density of the hot nuclei decreases faster in ^36Ar+^124Sn than in ^36Ar+^112Sn.
分 类 号:O571[理学—粒子物理与原子核物理]
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