## XMLSLZ(MTVTC)

#### Abstract

This table corresponds to the unified EoS of neutron star (npeµ) matter at zero temperature and β-equilibrium [XMLSL_2022], which is obtained in the framework of Thomas-Fermi approximation and assuming geometrical symmetries for the Wigner-Seitz cells [XSMLL_2022]. The covariant density functional MTVTC is adopted [MTVTC_2005].

Nparam | = | 1 |

Particles | = | npemN |

T min | = | 0.0 |

T max | = | 0.0 |

T pts | = | 1 |

nb min | = | 7.59e-11 |

nb max | = | 2.00e+00 |

nb pts | = | 1078 |

Y min | = | 0.0 |

Y max | = | 0.0 |

Y pts | = | 1 |

#### Nuclear Matter Properties

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

E_{0} |
= | 16.3 | Mev |

K | = | 239.8 | Mev |

K' | = | -513.0 | Mev |

J | = | 32.5 | Mev |

L | = | 89.6 | Mev |

K_{sym} |
= | -6.5 | MeV |

#### Neutron Star Properties

M_{max} |
= | 2.02 | M_{sun} |

MDU,e_{} |
= | 1.1 | M_{sun} |

R_{Mmax} |
= | 10.9 | km |

R_{1.4} |
= | 13.1 | km |

#### References

##### References to the original work:

- [XMLSL_2022] C.-J. Xia, T. Maruyama, A. Li, B. Y. Sun, W.-H. Long, and Y.-X. Zhang, Commun.Theor. Phys. 74, 095303 (2022)
- [XSMLL_2022] C.-J. Xia, B. Y. Sun, T. Maruyama, W.-H. Long, and A. Li, Phys. Rev. C 105, 045803 (2022)
- [MTVTC_2005] T. Maruyama, T. Tatsumi, D. N. Voskresensky, T. Tanigawa, and S. Chiba, Phys. Rev. C 72, 015802 (2005)

#### Data sheet

#### Data

eos.zip (0.17 MB) |

eos.zip_checksum.txt |

## Single files |

eos.t |

eos.nb |

eos.yq |

eos.thermo |

eos.compo |

eos.init |

eos.mr |