## GPPVA(FSU2H) NS unified inner crust-core

#### Abstract

This inner crust-core unified EoS for beta-equilibrium matter at zero temperature is constructed with a BPS outer crust [BPSA_1971] below baryon density of 0.002 fm^{âˆ’3}, an inner crust EoS [PFPR_2019], including nonspherical pasta phases, calculated within a self-consistent Thomas-Fermi approach [GPPVP_2014], and a homogeneous npe\mu core EoS, above baryon densit of 0.087 fm^{-3}. The EoS parameterisation used was the non-linear RMF FSU2H model [ NTCRD_2018].

Nparam | = | 1 |

Particles | = | None |

T min | = | 0.0 |

T max | = | 0.0 |

T pts | = | 1 |

nb min | = | 6.30e-12 |

nb max | = | 3.38e+00 |

nb pts | = | 282 |

Y min | = | 0.0 |

Y max | = | 0.0 |

Y pts | = | 1 |

#### Nuclear Matter Properties

n_{s} |
= | 0.1505 | fm^{-3} |

E_{0} |
= | -16.28 | Mev |

K | = | 238.0 | Mev |

K' | = | -24.6 | Mev |

J | = | 30.5 | Mev |

L | = | 44.5 | Mev |

K_{sym} |
= | 87.0 | MeV |

#### Neutron Star Properties

M_{max} |
= | 2.37 | M_{sun} |

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

R_{Mmax} |
= | 12.43 | km |

R_{1.4} |
= | 13.29 | km |

#### References

##### References to the original work:

- [GPPVP_2014] F. Grill, H. Pais, C. Providencia, I. Vidana and S. S. Avancini, Phys. Rev. C 90, 045803 (2014)
- [BPSA_1971] G. Baym, C. Pethick and P. Sutherland, Astrophys. J. 170, 299 (1971)
- [NTCRD_2018] R. Negreiros, L. Tolos, M. Centelles, A. Ramos, and V. Dexheimer, Astrophys. J. 863, 104 (2018)
- [PFPR_2019] C. ProvidÃªncia, M. Fortin, H. Pais, and A. Rabhi, Astron. Space Sci. 6, 13 (2019)

#### Data sheet

#### Data

eos.zip (0.13 MB) |

eos.zip_checksum.txt |

## Single files |

eos.init |

eos.nb |

eos.t |

eos.yq |

eos.thermo |

eos.mr |