arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2311.08092nucl-thhep-phnucl-ex
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热力学方法下$\boldsymbol{\rm \textbf{Au+Au}}$碰撞在$\boldsymbol{\rm \textbf{$\boldsymbol{\textbf{sqrt{s_{NN}}=}}$ 3 GeV}}$能量下的轻核产生:整体性质与集体流

Light Nuclei Production in Au+Au Collisions at $\sqrt{s_{NN}}=$ 3 GeV within Thermodynamical Approach: Bulk Properties and Collective Flow

M. Kozhevnikova, Yu. B. Ivanov

AI总结:

本研究用更新后的THESEUS模拟器结合热力学方法,模拟3 GeV能量下Au+Au碰撞的轻核产生,发现不同轻核适用不同冻出机制,验证了强子相对碰撞动力学的主导作用,良好重现了整体观测量与直接流数据。

摘要:

我们利用更新后的**THESEUS(基于三流体流体动力学的事件模拟器,由UrQMD(超相对论量子分子动力学)末态相互作用扩展)**,给出了碰撞能量为$\boldsymbol{\rm \textbf{$\boldsymbol{\textbf{sqrt{s_{NN}}=}}$ 3 GeV}}$$的Au+Au碰撞中轻核产生的模拟结果,并将结果与最新的STAR数据进行了对比。轻核产生在热力学方法框架下与强子同等处理。与轻核相关的唯一额外参数是晚冻出的能量密度,该参数模拟碰撞的后燃器阶段,因为轻核不参与UrQMD演化。研究发现,晚冻出更适用于氘核、氚核和$^3$He;值得注意的是,$^4$He的观测量用标准冻出能更好地重现。这表明$^4$He核在后燃器阶段存活得更好,因为它们是空间上更紧凑、束缚更紧密的物体,这是支持对轻核进行动力学处理的一个论据。模拟表明,碰撞动力学由强子相决定。计算结果显示,整体观测量和直接流的数据虽非完美但得到了良好重现,椭圆流则表现得更为复杂。

英文摘要:

We present results of simulations of light-nuclei production in Au+Au collisions at collision energy of $\sqrt{s_{NN}}=$ 3 GeV within updated Three-fluid Hydrodynamics-based Event Simulator Extended by UrQMD (Ultra-relativistic Quantum Molecular Dynamics) final State interactions (THESEUS). The results are compared with recent STAR data. The light-nuclei production is treated within the thermodynamical approach on equal basis with hadrons. The only additional parameter related to the light nuclei is the energy density of late freeze-out that imitates afterburner stage of the collision because the light nuclei do not participate in the UrQMD evolution. It is found that the late freeze-out is preferable for deuterons, tritons, and $^3$He. Remarkably, the $^4$He observables are better reproduced with the standard freeze-out. This suggests that the $^4$He nuclei better survive in the afterburner stage because they are more spatially compact and tightly bound objects. This is an argument in favor of dynamical treatment of light nuclei. The simulations indicate that the collision dynamics is determined by the hadronic phase. The calculated results reveal not perfect but a good reproduction of the data on bulk observables and directed flow. The elliptic flow turns out to be more intricate.

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