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- W2418582184 abstract "Upon application of the mass-density-dependent quark model with thermodynamic self-consistency, we investigate the bulk properties of hybrid stars and calculate the particle fraction and equation of state(EOS) for hybrid star matter. Numerical results indicate that the pressure extra term deriving from self-consistently thermodynamical treatment can soften the EOS, put off the appearence of phase transition and decrease the maximum mass for a hybrid star from 2.4(circle dot) (without pressure extra term) to 1.8M(circle dot) with corresponding radius from 15km to 12km. Similar to the Nambu-Jona-Lasinio(NJL) model, this model is suitable for describing the massive hybrid stars." @default.
- W2418582184 created "2016-06-24" @default.
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- W2418582184 date "2006-01-01" @default.
- W2418582184 modified "2023-09-24" @default.
- W2418582184 title "Mass-density-dependent quark model with thermodynamic self-consistency and hybrid stars" @default.
- W2418582184 hasPublicationYear "2006" @default.
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