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Chemical freeze-out parameters in Beam Energy Scan Program of STAR at RHIC

机译:在RHIC的星光能量扫描程序中的化学冻结参数

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The STAR experiment at RHIC has completed its first phase of the Beam Energy Scan (BES-I) program to understand the phase structure of the quantum chromodynamics (QCD). The bulk properties of the system formed in Au+Au collisions at different center of mass energy {formula} = 7.7, 11.5, 19.6, 27, and 39 GeV have been studied from the data collected in the year 2010 and 2011. The centrality and energy dependence of mid-rapidity (|y| < 0.1) particle yields, and ratios are presented here. The chemical freeze-out parameters are extracted using measured particle ratios within the framework of a statistical model.
机译:RHIC的恒星实验已经完成了光束能量扫描(BES-I)程序的第一阶段,以了解量子色能(QCD)的相位结构。在2010年和2011年的数据收集的数据中研究了在不同质量能量中心(公式} = 7.7,11.5,19.6,27和39 GEV的Au + Au碰撞中的系统的堆积性质。这里给出了中快度(| y | <0.1)颗粒产率的能量依赖性和比率。在统计模型的框架内使用测量的粒子比提取化学冻除参数。

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