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arXiv · 2310.17719

Quark stars in $D_3$-$D_7$ holographic model

M. Aleixo·C. H. Lenzi·W. de Paula·R. da Rocha
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Abstract

This work investigates static and dynamical quark star properties within a $D_3-D_7$ holographic model. We solve the Tolman-Oppenheimer-Volkoff equations for the quark matter equation of state obtained from the brane configuration. We determine the mass-radius diagram for a range of model parameters and compare with recent NICER observational data for the pulsars PSR J$0030+0451$ and PSR J$0740+6620$. Motivated by the GW170817 event detected by the LIGO-Virgo collaboration, we also calculate the tidal deformability parameter obtained for each component of the binary star system. We show that quark stars composed of flavor-independent quark matter derived from the $D_3-D_7$ holographic model are not able to satisfy simultaneously the LIGO-Virgo and NICER astrophysical bounds.

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M. Aleixo, C. H. Lenzi, W. de Paula, R. da Rocha. 2023-10-26. Quark stars in $D_3$-$D_7$ holographic model. https://doi.org/10.1140/epjc%2Fs10052-024-12619-7

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