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arXiv 1408.0495nucl-exhep-exhep-lathep-phnucl-th
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STAR净质子分布累积量的基线

Baseline for the cumulants of net-proton distributions at STAR

Xiaofeng Luo, Bedangadas Mohanty, Nu Xu

摘要:

我们提出了一个系统的比较最近测量的净质子分布的累积量之间的STAR 0-5%的中心金+金碰撞在$\sqrt{s_{NN}}$ =7.7-200 GeV和两种可能的基线措施,泊松和二项式基线。这些基线测量假设质子和反质子分布独立地遵循泊松统计或二项式统计。高阶累积净质子数据观察到偏离所有的基线测量研究在19.6和27 GeV。我们还比较了UrQMD和AMPT模型中的净质子涨落和净重子涨落,并利用一组公式将AMPT模型中的净质子涨落转换为净重子涨落。

英文摘要:

We present a systematic comparison between the recently measured cumulants of the net-proton distributions by STAR for 0-5% central Au+Au collisions at $\sqrt{s_{NN}}$=7.7-200 GeV and two kinds of possible baseline measures, the Poisson and Binomial baselines. These baseline measures are assuming that the proton and anti-proton distributions independently follow Poisson statistics or Binomial statistics. The higher order cumulant net-proton data are observed to deviate from all the baseline measures studied at 19.6 and 27 GeV. We also compare the net-proton with net-baryon fluctuations in UrQMD and AMPT model, and convert the net-proton fluctuations to net-baryon fluctuations in AMPT model by using a set of formula.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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