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Chiral model approach to quark matter nucleation in neutron stars

2012/01/11 by Domenico Logoteta, Ignazio Bombaci, Constança Providência +2
Earth and Planetary Sciences · Physics and Astronomy · #Cold Atom Physics and Bose-Einstein Condensates #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research #nucl-th

paper · pdf · doi:10.1103/physrevd.85.023003

published as Physical Review D 85, 023003 (2012)

openalex publication_date 2012/01/11 · arxiv created 2012/03/19 · arxiv updated 2012/03/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The nucleation process of quark matter in both cold and hot dense hadronic matter is investigated using a chiral approach to describe the quark phase. We use the Nambu--Jona--Lasinio and the chromo dielectric models to describe the deconfined phase and the nonlinear Walecka model for the hadronic one. The effect of hyperons on the transition phase between hadronic and quark matter is studied. The consequences of the nucleation process for neutron star physics are outlined.

Citations