## OPGR(GM1Y4) (with hyperons)

#### Abstract

This EoS is the classical RMF parameterisation GM1 [GMPR_1991] for cold neutron star matter in beta-equilibrium containing the baryon octet and electrons, see Ref. [OPGR_2015] for details of the parameterisation of hyperonic interactions. For the crust, the EoS by Douchin and Haensel [DHA_2001] has been added below a density of nB = 10^{−3} fm^{−3}. Hadronic charge fraction and compositional information is available for the core only.

Nparam | = | 1 |

Particles | = | npeBs |

T min | = | 0.0 |

T max | = | 0.0 |

T pts | = | 1 |

nb min | = | 7.93e-15 |

nb max | = | 1.20e+00 |

nb pts | = | 303 |

Y min | = | 0.0 |

Y max | = | 0.0 |

Y pts | = | 1 |

#### Nuclear Matter Properties

n_{s} |
= | 0.0 | fm^{-3} |

E_{0} |
= | 0.0 | Mev |

K | = | 0.0 | Mev |

K' | = | 0.0 | Mev |

J | = | 0.0 | Mev |

L | = | 0.0 | Mev |

K_{sym} |
= | 0.0 | MeV |

#### Neutron Star Properties

M_{max} |
= | 0.0 | M_{sun} |

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

R_{Mmax} |
= | 0.0 | km |

R_{1.4} |
= | 0.0 | km |

#### References

#### Data sheet

#### Data

eos.zip (0.07 MB) |

eos.zip_checksum.txt |

## Single files |

eos.compo |

eos.init |

eos.nb |

eos.t |

eos.thermo |

eos.yq |