The Chiral Phase Transitions of Helical Matter
Shen-Song Wan, Marco Ruggieri

TL;DR
This paper investigates the phase transitions of helical quark matter, examining how net helicity influences chiral symmetry restoration, phase diagram structure, and fluctuations, including effects of rotation.
Contribution
It introduces a detailed thermodynamic analysis of helical matter using the quark-meson model, highlighting the impact of helicity on phase transitions and fluctuations.
Findings
Helical density lowers the critical temperature for chiral symmetry restoration.
Rotation enhances fluctuations of the helical density.
The phase diagram shifts with net helicity, affecting the critical endpoint location.
Abstract
We study the thermodynamics of helical matter, namely quark matter in which a net helicity, , is in equilibrium. Interactions are modeled by the renormalized quark-meson model with two flavors of quarks. Helical density is described within the grand-canonical ensemble formalism via a chemical potential, . We study the transitions from the normal quark matter and hadron gas to the helical matter, drawing the phase diagram at zero temperature. We study the restoration of chiral symmetry at finite temperature and show that the net helical density softens the transition, moving the critical endpoint to lower temperature and higher baryon chemical potential. Finally, we discuss briefly the effect of a rigid rotation on the helical matter, in particular on the fluctuations of , and show that these are enhanced by the rotation.
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