Quantum Phase Transitions in Dense QCD
Tetsuo Hatsuda, Kenji Maeda

TL;DR
This paper reviews the complex phase structure of QCD at finite temperature and density, focusing on quantum phase transitions like chiral symmetry breaking, deconfinement, and color superconductivity, with implications for heavy-ion collisions and neutron stars.
Contribution
It provides a comprehensive summary of the current understanding of QCD phase transitions, emphasizing symmetry aspects and potential connections to ultracold atom physics.
Findings
Different QCD phases characterized by distinct condensates
Quantum phase transitions linked to symmetry changes
Relevance to heavy-ion collisions and astrophysical objects
Abstract
Quantum chromodynamics (QCD) at finite temperature, , and quark chemical potential, , has a rich phase structure: at low and low , the Nambu-Goldstone (NG) phase with nearly massless pions is realized by the dynamical breaking of chiral symmetry through condensation of quark-anti-quark pairs, while, at low and high , a Fermi liquid of deconfined quarks is expected to appear as a consequence of asymptotic freedom. Furthermore, in such a cold quark matter, condensation of quark-quark pairs leads to the color superconductivity (CSC). At high for arbitrary , all the condensates melt away and a quark-gluon plasma (QGP) is realized. The experimental exploration of thermal phase transition from the NG phase to QGP is being actively pursued in ultrarelativistic heavy ion collisions at RHIC (Relativistic Heavy Ion Collider), and will be continued in the future…
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Taxonomy
TopicsHigh-Energy Particle Collisions Research · Quantum Chromodynamics and Particle Interactions · Cold Atom Physics and Bose-Einstein Condensates
