论文标题

高能核冲突中光核的化学冻结和Hyper-Triton化学冻结拼图的分辨率

Chemical freeze-out of light nuclei in high energy nuclear collisions and resolution of the hyper-triton chemical freeze-out puzzle

论文作者

Bugaev, K. A., Vitiuk, O. V., Grinyuk, B. E., Yakovenko, N. S., Zherebtsova, E. S., Sagun, V. V., Ivanytskyi, O. I., Savchenko, D. O., Bravina, L. V., Blaschke, D. B., Farrar, G. R., Kabana, S., Kuleshov, S. V., Nikonov, E. G., Taranenko, A. V., Zabrodin, E. E., Zinovjev, G. M.

论文摘要

我们介绍了用新型的强子共振气体模型获得的最新结果的摘要,该模型具有多组分硬核排斥,该模型扩展了以描述Hadrons和Light(Anti-tim-Hyper-)核的混合物。对于在碰撞能量$ \ sqrt {s_ {nn}} = 200 $ GEV和Alice At $ \ sqrt {s_ {s_ {nn}} = 2.76 $ tev的情况下,通过恒星在碰撞能量$ \ sqrt {s_ {nn}} = 200 $ GEV处测量的辐射核数据非常准确的描述。这里讨论的最引人注目的结果是,对于最可能的化学冻结场景,发现的参数使我们能够重现实验比的值$ s_3 $和$ \ overline {s} _3 $而无需安装。

We present a summary of the recent results obtained with the novel hadron resonance gas model with the multicomponent hard-core repulsion which is extended to describe the mixtures of hadrons and light (anti-, hyper-)nuclei. A very accurate description is obtained for the hadronic and the light nuclei data measured by STAR at the collision energy $\sqrt{s_{NN}} =200$ GeV and by ALICE at $\sqrt{s_{NN}} =2.76$ TeV. The most striking result discussed here is that for the most probable chemical freeze-out scenario for the STAR energy the found parameters allow us to reproduce the values of the experimental ratios $S_3$ and $\overline{S}_3$ without fitting.

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