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arXiv 0710.3629hep-phnucl-th
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超相对论性重离子碰撞中的夸克动力学复合和质子π比

Dynamical quark recombination in ultrarelativistic heavy-ion collisions and the proton to pion ratio

Alejandro Ayala, Mauricio Martinez, Guy Paic, G. Toledo Sanchez

摘要:

我们研究夸克的热复合作为一个功能的能量密度的演化过程中的重离子碰撞的数值模型,再现方面的QCD现象。我们发现,从一组自由夸克(或夸克和反夸克)开始,形成无色三夸克团簇的几率与形成无色夸克-反夸克团簇的几率不同,前者在临界能量密度处有一个急剧的跳跃,而后者从低能量密度域到高能量密度域平稳过渡.我们将其解释为具有能量密度的重子和介子产生的数量差异。我们使用这种方法来计算质子和π介子光谱在Bjorken的情况下,将这些概率的演变与能量密度,因此与适当的时间。从光谱,我们计算质子π比,并比较在最高的RHIC能量的数据。我们表明,对于一个标准的参数选择,这个比例达到1,虽然最大值是非常敏感的初始演化适当的时间。

英文摘要:

We study quark thermal recombination as a function of energy density during the evolution of a heavy-ion collision in a numerical model that reproduces aspects of QCD phenomenology. We show that starting with a set of free quarks (or quarks and antiquarks) the probability to form colorless clusters of three quarks differs from that to form colorless clusters of quark-antiquark and that the former has a sharp jump at a critical energy density whereas the latter transits smoothly from the low to the high energy density domains. We interpret this as a quantitative difference in the production of baryons and mesons with energy density. We use this approach to compute the proton and pion spectra in a Bjorken scenario that incorporates the evolution of these probabilities with energy density, and therefore with proper time. From the spectra, we compute the proton to pion ratio and compare to data at the highest RHIC energies. We show that for a standard choice of parameters, this ratio reaches one, though the maximum is very sensitive to the initial evolution proper time.

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