Chiral symmetry breaking in accelerating and rotating frames
Zhi-Bin Zhu, Hao-Lei Chen, Xu-Guang Huang
TL;DR
The paper tackles how acceleration and rotation affect chiral symmetry in QCD-like matter using low-energy effective models in non-inertial frames. It develops a formalism in Rindler coordinates, derives gap equations for NLσM and NJL models, and reveals a critical role for the renormalization scheme: subtracting Rindler vacuum leads to an acceleration-independent $T_c$ determined by the local Tolman-like temperature, while subtracting Minkowski vacuum yields acceleration-enhanced symmetry breaking. Extending to combined acceleration and rotation, the work identifies two restoration mechanisms—acceleration-induced thermalization and rotation-induced chemical potential effects—and shows the critical acceleration $a_c$ decreases with angular velocity $Ω$, with stronger rotation effects at larger radii. These findings illuminate the interplay between Unruh-like thermality and rotation in QCD-like matter and highlight foundational questions about vacuum interpretation in non-inertial settings.
Abstract
We study chiral symmetry breaking and restoration in accelerating and rotating frames using low-energy effective models. By analyzing the chiral condensate in Rindler coordinates, we show that different renormalization schemes lead to distinct conclusions in accelerating frame: the scheme with subtracting divergences in Rindler vacuum supports an acceleration-independent critical temperatures, while the other scheme with subtracting divergences in Minkowski vacuum suggests enhanced critical temperature. We further investigate system with both rotation and acceleration. We find that the critical acceleration (see definition in Section V) for chiral symmetry restoration decreases with angular velocity, indicating cooperative effects from acceleration-induced thermalization and rotation-induced effective chemical potential.
