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Strange quark matter in a chiral SU(3) quark mean field model

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arxiv hep-ph/0205251 v1 pith:O4TDZZBP submitted 2002-05-22 hep-ph

classification hep-ph
keywords quarkmatterstrangevectorchiralfieldmeanmodel
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We apply the chiral SU(3) quark mean field model to investigate strange quark matter. The stability of strange quark matter with different strangeness fraction is studied. The interaction between quarks and vector mesons destabilizes the strange quark matter. If the strength of the vector coupling is the same as in hadronic matter, strangelets can not be formed. For the case of beta equilibrium, there is no strange quark matter which can be stable against hadron emission even without vector meson interactions.

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  1. Probing up-down quark matter via gravitational waves

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    Up-down quark stars in the two-families scenario yield tidal deformabilities compatible with GW170817, constraining the effective bag constant to approximately 50 MeV/fm^3.

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