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

#### Abstract

This inner crust-core unified EoS for beta-equilibrium matter at zero temperature is constructed with the BsK22 outer crust EoS by Pearson et al [PCP_2018] below baryon density of 0.002 fm^{−3}, an inner crust EoS, 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 0.074 fm^{−3}. The EoS parameterisation used was the density-dependent RMF TW model [TW_1999].

Nparam | = | 1 |

Particles | = | npemN |

T min | = | 0.0 |

T max | = | 0.0 |

T pts | = | 1 |

nb min | = | 4.68e-10 |

nb max | = | 1.44e+00 |

nb pts | = | 418 |

Y min | = | 0.0 |

Y max | = | 0.0 |

Y pts | = | 1 |

#### Nuclear Matter Properties

n_{s} |
= | 0.153 | fm^{-3} |

E_{0} |
= | -16.25 | Mev |

K | = | 240.0 | Mev |

K' | = | -540.0 | Mev |

J | = | 32.8 | Mev |

L | = | 55.0 | Mev |

K_{sym} |
= | -125.0 | MeV |

#### Neutron Star Properties

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

MDU,e_{} |
= | N/A | M_{sun} |

R_{Mmax} |
= | 10.7 | km |

R_{1.4} |
= | 12.33 | 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)
- [TW_1999] Typel, S. and Wolter, H.H., Nucl. Phys. A656 ,331 (1999)
- [PCP_2018] J. M. Pearson, N. Chamel, A. Y. Potekhin, A. F. Fantina, C. Ducoin, A. K. Dutta, and S. Goriely, MNRAS 481, 2994 (2018)

#### 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 |

eos.compo |