论文标题

在大型强子撞机能量中,可能形成$ PP $,$ P $ -PB,XE-XE和PB-PB碰撞的完美液体的可能形成:一种颜色弦乐渗透方法

Possible Formation of a Perfect Fluid in $pp$, $p$-Pb, Xe-Xe and Pb-Pb Collisions at the Large Hadron Collider Energies: A Color String Percolation Approach

论文作者

Sahu, Dushmanta, Tripathy, Sushanta, Sahoo, Raghunath, Tiwari, Swatantra Kumar

论文摘要

等温可压缩性($κ_ {\ rm t} $)是一个重要的热力学观测,可提供有关系统偏离完美流体行为的信息。在这项工作中,我们首次估计了使用颜色弦乐渗透模型(CSPM)在高能量规格和核碰撞中形成的QCD物质的等温可压缩性,在此中,我们研究了$κ_ {\ rm t} $作为最终州带电粒子乘积和初始percoliation跨各种校正温度的$κ_ {\ rm t} $的变化。不同碰撞能量下不同碰撞系统的估计初始渗滤温度有助于我们在进化的初始阶段更好地了解系统。等温可压缩性与众所周知的流体的比较结果表明,在重离子碰撞中形成的物质可能是自然界中最接近的{\ it最接近的完美液体}。该估计值补充了重型离子碰撞实验中可能的QGP培养基对最小剪切粘度与熵密度比的众所周知的观察。带电粒子的假性密度的阈值,$ \ langle dn _ {\ rm ch}/dη\ rangle \ geq 20 $在最终的状态事件中,可以观察到在LHC Energies处寻找可能的QGP形成。

Isothermal compressibility ($κ_{\rm T}$) is an important thermodynamic observable which gives information about the deviation of a system from perfect fluid behavior. In this work, for the first time we have estimated the isothermal compressibility of QCD matter formed in high energy hadronic and nuclear collisions using color string percolation model (CSPM), where we investigate the change in $κ_{\rm T}$ as a function of final state charged particle multiplicity and initial percolation temperature across various collision species. The estimated initial percolation temperature for different collision systems at different collision energies helps us to have a better understanding of the system at the initial phase of evolution. The comparison of the CSPM results for isothermal compressibility with that for the well known fluids, indicates that the matter formed in heavy-ion collisions might be the {\it closest perfect fluid} found in nature. This estimation complements the well-known observation of minimum shear viscosity to entropy density ratio for a possible QGP medium created in heavy-ion collision experiments. A threshold of pseudorapidity density of charged particles, $\langle dN_{\rm ch}/dη\rangle \geq 20 $ in the final state event multiplicity is observed, after which one may look for a possible QGP formation at the LHC energies.

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