Charged pion condensation and color superconductivity phenomena in chirally asymmetric dense quark matter
T. G. Khunjua, K. G. Klimenko, R. N. Zhokhov

TL;DR
This study investigates how charged pion condensation persists in dense, chirally asymmetric quark matter even with color superconductivity, suggesting it remains a viable phase in extreme conditions like neutron stars and heavy ion collisions.
Contribution
It demonstrates that charged pion condensation is not suppressed by color superconductivity in chirally imbalanced dense quark matter, revealing a more complex phase structure.
Findings
Charged pion condensation persists despite color superconductivity.
Chiral imbalance does not hinder pion condensation at high densities.
Pion condensation remains viable in conditions relevant to heavy ion collisions and neutron stars.
Abstract
In this paper, the question of the influence of color superconductivity (CSC) on the formation of a phase with condensation of charged pions in dense chirally asymmetric quark matter is studied. We consider it within the framework of the massless NJL model with a diquark interaction channel at zero temperature, but in the presence of baryon , isospin , chiral and chiral isospin chemical potentials. It has been shown in the mean-field approximation that in the presence of chiral imbalance, when and/or , CSC phenomenon does not hinder the generation of charged pion condensation in dense quark matter even at largest baryon densities attainable in heavy ion collisions experiments and in cores of neutron stars and its mergers. So charged pion condensation in dense quark matter with chiral imbalance predicted earlier is not in a…
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Taxonomy
TopicsHigh-pressure geophysics and materials · Pulsars and Gravitational Waves Research · Rare-earth and actinide compounds
