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- W2610165105 abstract "A two-phase description of the quark--nuclear matter hybrid equation of state that takes into account the effect of excluded volume in both the hadronic and the quark-matter phases is introduced. The nuclear phase manifests a reduction of the available volume as density increases, leading to a stiffening of the matter. The quark-matter phase displays a reduction of the effective string tension in the confining density functional from available volume contributions. The nuclear equation of state is based upon the relativistic density-functional model DD2 with excluded volume. The quark-matter equation of state is based upon a quasiparticle model derived from a relativistic density-functional approach and will be discussed in greater detail. The interactions are decomposed into mean scalar and vector components. The scalar interaction is motivated by a string potential between quarks, whereas the vector interaction potential is motivated by higher-order interactions of quarks leading to an increased stiffening at high densities. As an application, we consider matter under compact star constraints of electric neutrality and $ensuremath{beta}$ equilibrium. We obtain mass-radius relations for hybrid stars that form a third family, disconnected from the purely hadronic star branch, and fulfill the $2text{ }text{ }{M}_{ensuremath{bigodot}}$ constraint." @default.
- W2610165105 created "2017-05-12" @default.
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- W2610165105 date "2017-09-26" @default.
- W2610165105 modified "2023-10-04" @default.
- W2610165105 title "Quark-nuclear hybrid star equation of state with excluded volume effects" @default.
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- W2610165105 doi "https://doi.org/10.1103/physrevd.96.056024" @default.
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