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CAN ONE EXTRACT SOURCE RADII FROM TRANSPORT THEORIES

机译:可以从运输理论中提取来源半径

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摘要

To know the space-time evolution of a heavy-ion reaction is of great interest, especially in cases where the measured spectra do not allow to ascertain the underlying reaction mechanism. In recent times it became popular to believe that the comparison of Hanbury-Brown-Twiss correlation functions obtained from classical or semiclassical transport theories, like Boltzmann-Uhling-Uhlenbeck (BUU), Quantum Molecular Dynamics (QMD), VENUS, RQMD or ARC, with experiments may provide this insight. It is the purpose of this article to show that this conjecture encounters serious problems. The models which are suited to be compared with the experiments at CERN and Brookhaven are not able to predict a correlation function. Any agreement with existing data has to be considered as accidental. The models suited for lower energies can in principle predict correlation functions. The systematic error may be too large to be of use as far as quantitative conclusions are concerned. (C) 1997 Elsevier Science B.V. [References: 23]
机译:知道重离子反应的时空演化非常重要,特别是在所测光谱无法确定潜在的反应机理的情况下。近年来,人们越来越相信从经典或半经典传输理论(例如Boltzmann-Uhling-Uhlenbeck(BUU),量子分子动力学(QMD),VENUS,RQMD或ARC)获得的Hanbury-Brown-Twiss相关函数的比较,实验可以提供这种见解。本文的目的是证明此推测遇到严重问题。适合与CERN和Brookhaven的实验进行比较的模型无法预测相关函数。与现有数据的任何协议都必须视为偶然的。适用于较低能量的模型原则上可以预测相关函数。就定量结论而言,系统误差可能太大而无法使用。 (C)1997 Elsevier Science B.V. [参考:23]

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