## GPPVA(FSU2) NS unified inner crust-core

#### Abstract

This inner crust-core unified EoS for beta-equilibrium matter at zero temperature is con- structed with a BPS outer crust [BPSA_1971] below baryon density of 0.002 fm^{−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 density of 0.054 fm^{−3}. The EoS parameterisation used was the non-linear RMF FSU2 model [CP_2014].

Nparam | = | 1 |

Particles | = | None |

T min | = | 0.0 |

T max | = | 0.0 |

T pts | = | 1 |

nb min | = | 6.30e-12 |

nb max | = | 2.10e+00 |

nb pts | = | 253 |

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' | = | -149.0 | Mev |

J | = | 37.6 | Mev |

L | = | 113.0 | Mev |

K_{sym} |
= | 25.0 | MeV |

#### Neutron Star Properties

M_{max} |
= | 2.07 | M_{sun} |

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

R_{Mmax} |
= | 12.08 | km |

R_{1.4} |
= | 13.89 | 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)
- [PFPR_2019] C. Providência, M. Fortin, H. Pais, and A. Rabhi, Astron. Space Sci. 6, 13 (2019)
- [CP_2014] W.-C. Chen and J. Piekarewicz, Phys. Rev. C 90, 044305 (2014)

#### 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 |

eos.compo |