Chiral phase transitions of helical matter

We study the thermodynamics of helical matter, namely quark matter in which a net helicity nH 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 mu H. 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 end point 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 nH, and show that these are enhanced by the rotation.

Automated summary

The study focuses on the thermodynamics of helical matter, specifically quark matter with a net helicity nH in equilibrium. Interactions are modeled using the renormalized quark-meson model with two quark flavors, with helical density described through grand-canonical ensemble formalism. The research also explores the transitions from normal quark matter and hadron gas to helical matter, drawing the phase diagram at zero temperature, and investigates the impact of rigid rotation on helical matter, particularly on the fluctuations of nH, which are enhanced by the rotation.