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Fragment formation in central heavy ion collisions at relativistic energies

机译:相对论能量在中心重离子碰撞中的碎片形成

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We perform a systematic study of the fragmentation path of excited nuclear matter in central heavy ion collisions at the intermediate energy of 0.4 A GeV. The theoretical calculations are based on a relativistic Boltzmann-Uehling-Uhlenbeck (RBUU) transport equation including stochastic effects. A relativistic mean field (RMF) approach is used, based on a non-linear Lagrangian, with coupling constants tuned to reproduce the high density results of calculations with correlations. At variance with the case at Fermi energies, a new fast clusterization mechanism is revealed in the early compression stage of the reaction dynamics. Fragments appear directly produced from phase space fluctuations due to two-body correlations. In-medium effects of the elastic nucleon-nucleon cross sections on the fragmentation dynamics are particularly discussed. The subsequent evolution of the primordial clusters is treated using a simple phenomenological phase space coalescence algorithm. The reliability of the approach, formation and recognition, is investigated in detail by comparing fragment momentum space distributions and simultaneously their yields with recent experimental data of the FOPI Collaboration by varying the system size of the colliding system, i.e., its compressional energy (pressure, radial flow). We find an excellent agreement between theory and experiment in almost all the cases and, on the other hand, some limitations of the simple coalescence model. Furthermore, the temporal evolution of the fragment structure is explored with a clear evidence of an earlier formation of the heavier clusters, that will appear as interesting relics of the high density phase of the nuclear equation of state (EoS). (c) 2005 Elsevier B.V. All rights reserved.
机译:我们对中心重离子碰撞在0.4 A GeV的中间能下激发核物质的碎裂路径进行了系统的研究。理论计算是基于相对论的玻耳兹曼-乌林-乌伦贝克(RBUU)输运方程,其中包括随机效应。基于非线性拉格朗日方法,使用相对论平均场(RMF)方法,并调整耦合常数以重现具有相关性的高密度计算结果。与费米能量的情况不同,在反应动力学的早期压缩阶段揭示了一种新的快速聚类机制。碎片似乎是由于两体相关性而由相空间波动直接产生的。特别讨论了弹性核子-核子横截面对断裂动力学的中等影响。使用简单的现象相空间合并算法处理原始簇的后续演化。通过比较碎片动量空间分布以及其产量与FOPI Collaboration的最新实验数据(通过改变碰撞系统的系统大小,即其压缩能(压力,压力,径向流)。在几乎所有情况下,我们都在理论和实验之间找到了极好的共识,另一方面,我们发现了简单合并模型的某些局限性。此外,研究了碎片结构的时间演变,并得到了较重聚类较早形成的明确证据,这些聚类将作为核态方程(EoS)高密度相的有趣文物出现。 (c)2005 Elsevier B.V.保留所有权利。

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