arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2106.04543nucl-thhep-ph
收藏

来自UrQMD的RHIC-BES能量的哈勃膨胀和冻结

Hubble Expansion and Freeze-Out at RHIC-BES Energies from UrQMD

Gabriele Inghirami, Tom Reichert, Marcus Bleicher

摘要:

重离子碰撞中的冻结过程是由散射率和物质膨胀率之间的竞争驱动的。我们分析的膨胀率$Θ$(通常称为哈勃流)在相对论重离子碰撞在FAIR和RHIC-BES的能量制度,并比较它的散射率$Γ$使用UrQMD传输模型。我们观察到,系统的时间演化被清楚地分为一个压缩阶段和一个膨胀阶段与时间相关的$Θ_\parallel$和$Θ_\perp$。哈勃膨胀在动力学解耦的计算值与以前的简单估计与统计强子化模型与西门子-拉斯穆森型发射源。然而,正如所料,膨胀物质的实际形状介于球对称和纯纵向膨胀之间。我们确认的第一次在微观模拟中,去耦超曲面确实是由竞争的膨胀率$Θ$和散射率$Γ$如前所述。这表明,在本研究中探索的碰撞能量范围内,简单的等温/等能量密度标准,通常用于混合模型耦合流体动力学和运输模拟可能无法捕获真正的解耦超曲面。

英文摘要:

The freeze-out process in heavy ion collisions is driven by the competition between the scattering rate and the expansion rate of the matter. We analyse the expansion rate $Θ$ (often called Hubble flow) in relativistic heavy ion collisions in the FAIR and RHIC-BES energy regimes and compare it to the scattering rate $Γ$ using the UrQMD transport model. We observe that the time evolution of the system is clearly separated into a compression phase and an expansion phase with time dependent $Θ_\parallel$ and $Θ_\perp$. The calculated values of the Hubble expansion at kinetic decoupling are in line with previous simple estimates by statistical hadronization models with a Siemens-Rasmussen type emission source. However, the actual shape of the expanding matter is, as expected, found to be between a spherically symmetric and a purely longitudinal expansion. We confirm for the first time in a microscopic simulation that the decoupling hypersurface is indeed determined by the competition of the expansion rate $Θ$ and the scattering rate $Γ$ as suggested previously. This suggests that, in the range of collision energies explored in this study, simple iso-thermal/iso-energy density criteria that are often used in hybrid models to couple hydrodynamic and transport simulations may not capture the true decoupling hyper-surface.

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。

↑