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首页> 外文期刊>Physical review, C >Nuclear system size scan for freeze-out properties in relativistic heavy-ion collisions by using a multiphase transport model
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Nuclear system size scan for freeze-out properties in relativistic heavy-ion collisions by using a multiphase transport model

机译:使用多相输送模型,核系统尺寸扫描相对论重离子碰撞中的冻结性质

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摘要

A system size scan program was recently proposed for the STAR experiments at the Relativistic Heavy Ion Collider (RHIC). In this study, we employ a multiphase transport (AMPT) model for considering the bulk properties at the freeze-out stage for B-10 + B-10, C-12 + C-12, O-16+ O-16, Ne-20 Ne-20, Ca-40 Ca-40, Zr-96 + Zr-96, and Au-197 Au-197 collisions at RHIC energies root s(NN) of 200, 20, and 7.7 GeV. The results for Au-197 Au-197 collisions are comparable with those of previous experimental STAR data. The transverse momentum P T spectra of charged particles (pi(+/- ), K-+/-, p, and (p) over bar) at the kinetic freeze-out stage, based on a blast-wave model, are also discussed. In addition, we use a statistical thermal model to extract the parameters at the chemical freeze-out stage, which agree with those from other thermal model calculations. It was found that there is a competitive relationship between the kinetic freeze-out parameter T-kin and the radial expansion velocity beta(T), which also agrees with the STAR or ALICE results. We found that the chemical freeze-out strangeness potential mu(s) remains constant in all collision systems and that the fireball radius R is dominated by < N-part >, which can be well fitted by a function of a < N-part >(b) with b approximate to 1/3. In addition, we calculated the nuclear modification factors for different collision systems with respect to the B-10 + B-10 system, and found that they present a gradual suppression within a higher P T range from small to large systems.
机译:最近提出了一种系统尺寸扫描程序,用于在相对论的重离子撞机(RHIC)处的明星实验。在这项研究中,我们采用多相传输(AMPT)模型,用于考虑B-10 + B-10,C-12 + C-12,O-16 + O-16,NE的冻结阶段的散装性能-20NE-20,CA-40 CA-40,ZR-96 + ZR-96,ZR-96 + ZR-96和AU-197 AU-197在200,20和7.7 GEV的RHIC Energies Roots S(NN)的碰撞。 AU-197 AU-197碰撞的结果与先前的实验恒星数据的结果相当。还讨论了基于冲击波模型的动力学冻退出阶段的带电粒子(PI(+/-),K - + / - ,P和(P)的PI(+/-),K - + / - ,P和(P))的横向动量Pt光谱。此外,我们使用统计热模型提取化学冻除出阶段的参数,这与来自其他热模型计算的液位同意。发现动力学冻结参数T-Kin与径向膨胀速度β(T)之间存在竞争关系,这也同意恒星或Alice结果。我们发现,在所有碰撞系统中,化学冻结奇怪潜在MU保持恒定,并且火球半径r由 (b)b近1/3近似。此外,我们计算了与B-10 + B-10系统的不同碰撞系统的核修改因子,发现它们在从小到大系统的较高P T范围内呈现逐渐抑制。

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