Resonance suppression during the hadronic stage from the FAIR to the intermediate RHIC energy regime

Amine Chabane, Lisa Engel, Tom Reichert, Jan Steinheimer, Marcus Bleicher
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Abstract

The energy and centrality dependence of the kaon resonance ratio $(K^{*0}+\Bar{K}^{*0})/(K^+ + K^-)$ is explored in the RHIC-BES and CBM-FAIR energy regime. To this aim, the Ultra-relativistic Quantum Molecular Dynamics (UrQMD) model is employed to simulate reconstructable $K^{*}$ resonances in Au+Au and p+p collisions from $\sqrt{s_{\text{NN}}}=3-39$ GeV. We obtain a good description of the resonance yields and mean transverse momenta over the whole investigated energy range. The decrease of the $K^*/K$ ratio, with increasing centrality is in line with the available experimental data. We also observe the experimenatlly measured increase in $\langle p_{\text{T}}\rangle$ with increasing centrality which is interpreted as a lower reconstruction probability of low-$p_{\text{T}}$ $K^*$ due to the $p_{\text{T}}$ dependent absorption of the decay daughter hadrons. We conclude that the observed suppression of reconstructable $K^{*}$ resonances provides a strong sign of an extended hadronic rescattering stage at all investigated energies. Its duration increases from peripheral to central reactions as expected. Following a method, suggested by the STAR experiment, the "duration" of the hadronic stage is extracted using the $K^*/K$ ratios at chemical and kinetic freeze-out. The resulting lifetimes are in good agreement with the experimental data, but much shorter than the actual lifetime of the hadronic phase in the transport simulation. This indicates that the experimental method to estimate the life time of the hadronic stage is too simplified.
从 FAIR 到中级 RHIC 能量机制的强子阶段的共振抑制
在RHIC-BES和CBM-FAIR能级体系中探索了高子共振比$(K^{*0}+\Bar{K}^{*0})/(K^+ + K^-)$ 的能量和中心性依赖性。为此,我们使用超相对论量子分子动力学(UrQMD)模型模拟了Au+Au和p+p碰撞中从$\sqrt{s_{text/{NN}}=3-39$ GeV的可重构$K^{*}$共振。我们获得了整个研究能量范围内共振产率和平均横坐标矩的良好描述。随着中心性的增加,K^*/K$比值的下降与现有的实验数据相符。我们还观察到,在中心度增加的过程中,实验测得的$/角p_{text{T}}/rangle$增加了,这被解释为由于衰变子强子对$p_{text{T}}$的依赖性吸收,低$p_{text{T}}$ $K^*$的重建概率降低了。我们的结论是,观测到的可重构$K^{*}$共振的抑制提供了一个强烈的信号,表明在所有被研究的能量下,强子再散射阶段都在延长。正如预期的那样,它的持续时间从外围反应到中心反应都在增加。根据 STAR 实验提出的一种方法,利用化学和动力学冻结时的 $K^*/K$ 比率来提取强子阶段的 "持续时间"。得出的寿命与实验数据十分吻合,但比转运模拟中强子阶段的实际寿命短得多。这表明估计强子阶段寿命的实验方法过于简化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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