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arXiv · 2009.14079

Holographic quark matter with colour superconductivity and a stiff equation of state for compact stars

Kazem Bitaghsir Fadafan·Jesus Cruz Rojas·Nick Evans
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Abstract

We present a holographic model of QCD with a first order chiral restoration phase transition with chemical potential, mu. The first order behaviour follows from allowing a discontinuity in the dual description as the quarks are integrated out below their constituent mass. The model predicts a deconfined yet massive quark phase at intermediate densities (350 MeV< mu <500 MeV), above the nuclear density phase, which has a very stiff equation of state and a speed of sound close to one. We also include a holographic description of a colour superconducting condensate in the chirally restored vacuum and study the resulting equation of state. They provides a well behaved first order transition from the deconfined massive quark phase at very high density (mu>500 MeV). We solve the Tolman-Oppenheimer-Volkoff equations with the resulting equations of state and find stable hybrid stars with quark cores. We compute the tidal deformability for these hybrid stars and show they are consistent with LIGO/Virgo data on a neutron star collision. Our holographic model shows that quark matter could be present at the core of such compact stars.

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Kazem Bitaghsir Fadafan, Jesus Cruz Rojas, Nick Evans. 2020-09-29. Holographic quark matter with colour superconductivity and a stiff equation of state for compact stars. https://doi.org/10.1103/physrevd.103.026012

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