# Compact Star of Holographic Nuclear Matter and GW170817

## TL;DR

This paper employs a holographic QCD model to derive a nuclear matter equation of state, enabling the modeling of compact stars and matching gravitational wave data from GW170817.

## Contribution

It introduces a novel holographic approach to nuclear matter, providing an equation of state that aligns with observational data from gravitational wave events.

## Key findings

- The EoS satisfies causality and exceeds the sound barrier.
- Predicted star properties match GW170817 data.
- The model yields realistic star compactness and tidal deformability.

## Abstract

We use a holographic model of quantum chromodynamics to extract the equation of state (EoS) for the cold nuclear matter of moderate baryon density. This model is based on the Sakai-Sugimoto model in the deconfined Witten's geometry with the additional point-like D4-brane instanton configuration as the holographic baryons. Our EoS takes the following doubly-polytropic form: $ \epsilon=2.629 {\cal A}^{-0.192} p^{1.192}+0.131 {\cal A}^{0.544} p^{0.456}$ with $\cal A$ a tunable parameter of order $10^{-1}$, where $\epsilon$ and $p$ are the energy density and pressure, respectively. The sound speed satisfies the causality constraint and breaks the sound barrier. We solve the Tolman-Oppenheimer-Volkoff equations for the compact stars and obtain the reasonable compactness for the proper choices of $\cal A$. Based on these configurations we further calculate the tidal deformability of the single and binary stars. We find our results agree with the inferred values of LIGO/Virgo data analysis for GW170817.