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Validity of reducing dynamical degrees of freedom in the coupled n–σ system under limited scale separation

Ascertain whether, in heavy-ion collision scenarios where scale separation is limited, one can consistently reduce dynamical degrees of freedom in the coupled chiral condensate–baryon density (n–σ) system—such as integrating out the σ field as a fast mode—without losing essential physics relevant to critical fluctuations.

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Background

Many studies simplify the dynamics near the QCD critical point by treating σ as a fast mode and focusing on conserved-charge diffusion (model B). However, heavy-ion collisions feature short lifetimes and comparable microscopic and macroscopic time scales, which may invalidate such reductions.

Clarifying when (or if) the σ degree of freedom can be safely eliminated is essential for constructing reliable dynamical frameworks that capture critical phenomena in realistic collision conditions.

References

However, as already discussed, the scale separation is not well established in the heavy-ion collisions. It remains nontrivial whether we may reduce a dynamical degree in the equations of motion for the coupled n–σ system in the context of heavy-ion collisions.

Dynamical evolution of critical fluctuations with second-order baryon diffusion coupled to chiral condensate (2502.17791 - Sakai et al., 25 Feb 2025) in Section I: Introduction