Kaon condensation in the quark-meson coupling model and compact stars

Abstract

The properties of neutron stars constituted of a crust of hadrons and an internal part of hadrons and kaon condensate are calculated within the quark-meson-coupling model. We have considered stars with nucleons only in the hadron phase and also stars with hyperons as well. The results are compared with the ones obtained from the non-linear Walecka model for the hadronic phase.

arXiv comment10 pages, 6 figures

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Cited by in corpus (27)

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• Quark-Meson-Coupling (QMC) model for finite nuclei, nuclear matter and beyond
• Quark stars within relativistic models
• Constraining strangeness in dense matter with GW170817
• Evolution of proto-neutron stars with the hadron-quark phase transition
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• How the HESS J1731-347 event could be explained using ${\mathbf{K}}^{-}$ condensation
• Effects of the symmetry energy on the kaon condensates in the QMC Model
• Kinetic approach to a relativistic Bose-Einstein condensate
• Metastable pions in dense media
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• Particle Production within the Quark Meson Coupling Model
• Rotating compact star with superconducting quark matter
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