Mixed phases of compact star matter in a unified mean-field approach
Cheng-Jun Xia, Toshiki Maruyama, Nobutoshi Yasutake, Toshitaka Tatsumi

TL;DR
This paper uses an extended NJL model to study mixed phases in dense stellar matter, revealing geometric structures during phase transitions and their implications for understanding compact star cores.
Contribution
It introduces a unified mean-field approach to analyze various first-order phase transitions in dense matter, incorporating complex geometries and interactions.
Findings
Geometrical structures appear in liquid-gas and deconfinement transitions.
No geometrical structures are found for chiral phase transitions.
Attractive interactions between strange quark matter and hyperons are observed.
Abstract
Based on an extended NJL model that treats baryons as clusters of quarks, we investigate the properties and microscopic structures of mixed phases for various types of first-order phase transitions in a unified manner, where the model parameters are fixed by reproducing nuclear matter properties and the binding energies of finite nuclei. In particular, based on the Thomas-Fermi approximation, we investigate the mixed phases arise from the liquid-gas phase transition of nuclear matter, chiral phase transition, and deconfinement phase transition in dense stellar matter adopting spherical and cylindrical approximations for the Wigner-Seitz cells. It is found that the geometrical structures do not emerge for chiral phases transition, while the droplet, rod, slab, tube, and bubble phases emerge sequentially as density increases for the liquid-gas and deconfinement phase transitions.…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
