Finite Size Scaling in Time Evolution During the Colorless-QCD Confining Phase Transition
The time evolution of the expanding Colorless Partonic Matter, created in Ultra-Relativistic Heavy Ion Collisions and undergoing the confining phase transition towards a Hadronic Gas, is discussed in the context of a unified model combining our Colorless QCD-MIT Bag Model with the boost invariant Bj...
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Zusammenfassung: | The time evolution of the expanding Colorless Partonic Matter, created in
Ultra-Relativistic Heavy Ion Collisions and undergoing the confining phase
transition towards a Hadronic Gas, is discussed in the context of a unified
model combining our Colorless QCD-MIT Bag Model with the boost invariant
Bjorken expansion. The Bjorken Equation in the case of a longitudinal expansion
scenario of a non-ideal relativistic medium in finite volume is solved using
certain initial conditions $(\tau_i,T(\tau_i))$ and their effect is studied in
detail. The evolution of the temperature as a function of the proper time
$T(\tau,V)$ is then obtained at different volumes. Different times
characterising different scales of the whole time evolution, like the time of
the finite volume transition point $\tau_0(V)$, the hadronic time $\tau_H(V)$
at which the hadronization is completed, the lifetime of the Colorless Partonic
Plasma $\Delta \tau_{CPP}(V)$ and the lifetime of the confining phase
transition $\Delta \tau_{PT}(V)$ are calculated and their finite size scaling
properties are studied in detail. New finite size scaling laws are derived.
Also, the time evolution of some Thermal Response Functions as the order
parameter $\mathcal{H}(\tau,V)$, energy density $\epsilon(\tau,V)$, pressure
$\mathscr{P}(\tau,V)$ and the sound velocity $\mathscr{C}_{s}(\tau,V)$ are
investigated and studied in detail. We find that the time evolution of our
system is really affected by the colorlessness requirement and the initial
conditions of the partonic matter: the closer the volume is to the
thermodynamic limit, the longer are the times and the lifetimes of the system.
A detailed analysis of the temporal decreasing, in negative power, of the
energy density $\epsilon(\tau,V) \propto \tau^{-\theta}$ in each of the three
stages of the Bjorken expansion is carried out. |
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DOI: | 10.48550/arxiv.1909.05668 |