## GPPVA(DDME2) NS crust

#### Abstract

This inner crust EoS, including nonspherical pasta phases, was calculated within a self- consistent Thomas-Fermi approach [GPPVP_2014] for beta-equilibrium matter at zero temperature. This EoS was published in Ref. [GPPVP_2014]. The EoS parameterisation used was the density- dependent RMF DDME2 model [LNVR_2005]. For the outer crust, the BsK22 EoS by Pearson et al [PCP_2018] was added below baryon density of 0.002 fm^{−3}.

Nparam | = | 1 |

Particles | = | npeN |

T min | = | 0.0 |

T max | = | 0.0 |

T pts | = | 1 |

nb min | = | 4.68e-10 |

nb max | = | 7.20e-02 |

nb pts | = | 288 |

Y min | = | 0.0 |

Y max | = | 0.0 |

Y pts | = | 1 |

#### Nuclear Matter Properties

n_{s} |
= | 0.152 | fm^{-3} |

E_{0} |
= | -16.14 | Mev |

K | = | 251.0 | Mev |

K' | = | 479.0 | Mev |

J | = | 32.3 | Mev |

L | = | 51.0 | Mev |

K_{sym} |
= | -87.2 | MeV |

#### Neutron Star Properties

M_{max} |
= | 2.488 | M_{sun} |

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

R_{Mmax} |
= | 12.15 | km |

R_{1.4} |
= | 13.23 | 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)
- [LNVR_2005] G. A. Lalazissis, T. Niksic, D. Vretenar, and P. Ring, Phys. Rev. C 71, 024312 (2005)
- [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 |