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The QCD Kondo phase in quark stars

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arxiv 1901.01623 v2 pith:7I475M2A submitted 2019-01-06 nucl-th hep-lathep-ph

R. Fariello , Juan C. Macías , F. S. Navarra This is my paper · ORCID
classification nucl-thhep-lathep-ph
keywords kondophasequarkstarsimpuritiesmatteraddedcharm
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We study light (u, d) quark matter with charm impurities. These impurities are added to the Lagrangian density. We derive the equation of state (EOS) of this kind of quark matter, which contains a Kondo phase. We explore this EOS and study the structure of stars, identifying the effects of the Kondo phase. Solving the TOV equations and computing the mass-radius diagram, we find that the presence of a Kondo phase leads to smaller and lighter stars.

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Cited by 1 Pith paper

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  1. Cold quark matter with heavy quarks and the stability of charm stars

    hep-ph 2019-08 conditional novelty 6.0 of 10

    Cold, beta-equilibrated charm quark matter from perturbative QCD yields charm star configurations that are dynamically unstable under radial oscillations.

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