Λ和Λ¯Au+Au碰撞中的冻结分布和全局极化

Nikita Tsegelnik, E. Kolomeitsev, V. Voronyuk
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引用次数: 1

摘要

在PHSD输运模型中模拟了sNN=7.7和11.5 GeV下的金-金碰撞。在每次碰撞事件中,旁观者核子被分离,参与者的流化过程被执行。在朗道坐标系中确定了局部速度,计算了运动涡场和热涡场。我们分析了Λs和Λ¯s产生或最后相互作用的细胞的热力学性质。这些细胞有助于形成观测到的由介质热涡度诱导的超子的全局极化。发现Λ¯极化信号主要由碰撞早期的高温、密集和高涡度的单体决定,而Λ极化信号则是在较长时间内积累的,包括涡度较低的单体。在sNN=11.5 GeV能量下,计算出的Λs和Λ¯s的全局极化与STAR合作的实验结果吻合得很好。对于sNN=7.7 GeV的碰撞,我们可以重现Λ超子的STAR数据,但明显低估了Λ¯的观测到的全局极化。此外,我们还考虑了7.7 GeV碰撞中超子极化的中心依赖性。它随着中心性的增加而增加,在65-75%时达到最大值,然后在外围碰撞时开始迅速下降。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Λ and Λ¯ Freeze-Out Distributions and Global Polarizations in Au+Au Collisions
The gold–gold collisions at sNN=7.7 and 11.5 GeV are simulated within the PHSD transport model. In each collision event, the spectator nucleons are separated and the fluidization procedure for the participants is performed. The local velocities are determined in the Landau frame and the kinematic and thermal vorticity fields are evaluated. We analyze the thermodynamic properties of the cells where Λs and Λ¯s were born or had their last interaction. Such cells contribute to the formation of the observed global polarization of hyperons induced by the thermal vorticity of the medium. The Λ¯ polarization signal is found to be mainly determined by hot, dense, and highly vortical cells at the earlier stage of the collision, whereas the Λ polarization signal is accumulated over the longer time and includes cells with lower vorticity. The calculated global polarizations for both Λs and Λ¯s agree well with the experimental finding by the STAR collaboration at energy sNN=11.5 GeV. For collisions at sNN=7.7 GeV, we can reproduce the STAR data for Λ hyperons, but significantly underpredict the observed global polarization of Λ¯. Furthermore, we consider the centrality dependence of the hyperon polarization in collisions at 7.7 GeV. It increases with an increase of centrality, reaches a maximum at 65–75% and then starts decreasing rapidly for peripheral collisions.
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