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Hybrid stars with color superconductivity within a nonlocal chiral quark model

H. Grigorian·D. Blaschke·D. N. Aguilera
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Abstract

The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation. Special emphasis is on the occurrence of a diquark condensate which signals a phase transition to color superconductivity and its effects on the equation of state. We present a fit formula for the Bag pressure, which is density dependent in case when the quark matter is color superconducting. We calculate the quark star configurations by solving the Tolman- Oppenheimer- Volkoff equations and demonstrate the effects of diquark condensation on the stability of hybrid stars for different formfactors of the quark interaction.

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H. Grigorian, D. Blaschke, D. N. Aguilera. 2004-03-07. Hybrid stars with color superconductivity within a nonlocal chiral quark model. https://doi.org/10.1103/physrevc.69.065802

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