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arXiv 2305.02487nucl-th
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基于聚并模型的$\u221as_{NN}=3$ GeV下Au+Au碰撞中的轻核产生

Light nuclei production in Au+Au collisions at $\sqrt{s_{NN}}=3$ GeV from coalescence model

Yue Xu, Xionghong He, Nu Xu

AI总结:

本研究基于核子聚并模型,利用JAM输运模型结合后处理聚并模块研究3 GeV质心系能量下Au+Au碰撞中的轻核产生,通过扫描聚并参数重现实验谱,揭示了参数与轻核结合能、直径的潜在关联。

摘要:

核子聚并模型是高能重离子碰撞中轻核产生最常用的理论模型之一。本文利用输运模型JAM结合简化的后处理聚并模块,研究了质心系能量$\u221as_{NN}=3$ GeV的Au+Au碰撞中轻核$d$、$t$、$^{3}$He和$^{4}$He的产生过程。我们扫描了核子聚并形成轻核的唯象聚并参数截断值,即相对空间距离$ΔR$和动量差$ΔP$,以重现STAR实验测量的轻核$p_{\ m T}$谱。结果表明,聚并参数与这些轻核的结合能以及直径之间存在潜在关联。

英文摘要:

The nucleon coalescence model is one of the most popular theoretical models for light nuclei production in high-energy heavy-ion collisions. The production of light nuclei $d$, $t$, $^{3}$He, and $^{4}$He is studied using the transport model JAM with a simplified afterburner coalescence at $\sqrt{s_{NN}}=3$ GeV Au+Au collisions. We scan the cut-off of phenomenological coalescence parameters, the relative spatial distance $ΔR$ and momentum difference $ΔP$, for formation of light nuclei by nucleon coalescence to reproduce the light nuclei $p_{\rm T}$ spectra measured by STAR experiment. The results indicate a potential connection between the coalescence parameters and the binding energy as well as the diameter of these light nuclei.

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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