## JJ(VQCD(APR)), intermediate

#### Abstract

These EoSs (soft, intermediate, and stiff variants) are mostly based on gauge/gravity duality and include both nuclear and quark matter phases. They were selected as representative examples from a larger family of EoSs constructed in [JJNR_2021]. EoSs of this type were first considered in [ EJNS_2020]. They use the APR EoS [APRP_1989] for nuclear matter at low densities, and the holographic V-QCD model for dense nuclear matter [ IJN_2019] as well as for quark matter [JJR_2019]. To be precise, the EoSs are those considered in [JJNR_2021] with APR low density EoS, matching density of 1.6 times the saturation density, and V-QCD with potentials 5b, 7a, and 8b for the the soft, intermediate, and stiff variants, respectively.

Nparam | = | 1 |

Particles | = | npeNq |

T min | = | 0.0 |

T max | = | 0.0 |

T pts | = | 1 |

nb min | = | 1.00e-12 |

nb max | = | 9.99e+00 |

nb pts | = | 651 |

Y min | = | 0.0 |

Y max | = | 0.0 |

Y pts | = | 1 |

#### Nuclear Matter Properties

n_{s} |
= | 0.0 | fm^{-3} |

E_{0} |
= | 0.0 | Mev |

K | = | 0.0 | Mev |

K' | = | 0.0 | Mev |

J | = | 0.0 | Mev |

L | = | 0.0 | Mev |

K_{sym} |
= | 0.0 | MeV |

#### Neutron Star Properties

M_{max} |
= | 0.0 | M_{sun} |

MDU,e_{} |
= | 0.0 | M_{sun} |

R_{Mmax} |
= | 0.0 | km |

R_{1.4} |
= | 0.0 | km |

#### References

##### References to the original work:

- [APRP_1998] A. Akmal, V. R. Pandharipande and D. G. Ravenhall, Phys. Rev. C 58, 1804 (1998)
- [JJR_2019] N. Jokela, M. Jarvinen and J. Remes, JHEP 03, 041 (2019)
- [IJN_2019] T. Ishii, M. Jarvinen and G. Nijs, JHEP 07, 003 (2019)
- [EJNS_2020] C. Ecker, M. Jarvinen, G. Nijs and W. van der Schee, Phys. Rev. D 101, 103006 (2020)
- [JJNR_2021] N. Jokela, M. Jarvinen, G. Nijs and J. Remes, Phys. Rev. D 103, 086004 (2021)

#### Data sheet

#### Data

eos.zip (0.14 MB) |

eos.zip_checksum.txt |

## Single files |

eos.init |

eos.nb |

eos.t |

eos.yq |

eos.thermo |

eos.mr |