## SFH(SFHx) neutron matter (no electrons)

#### Abstract

This is the zero electron faction EOS table with RMF interactions SFHx [SHF_2013]. Contributions of neutrons, anti-neutrons, protons, and anti-protons are included, whereas the net abundance of protons is always zero. The details of the underlying EOS model at finite Y e can be found in Ref. [HSNP_2010], where the TMA interactions were used. The manual from this web page gives further information about the table. Applications of HS EOS for various different RMF interactions in supernova simulations can be found in Refs. [SHF_2013,HFSLA_2012].

Nparam | = | 2 |

Particles | = | np N |

T min | = | 1.00e-01 |

T max | = | 1.58e+02 |

T pts | = | 81 |

nb min | = | 1.00e-12 |

nb max | = | 1.00e+01 |

nb pts | = | 326 |

Y min | = | 0.0 |

Y max | = | 0.0 |

Y pts | = | 1 |

#### Nuclear Matter Properties

n_{s} |
= | 0.1455 | fm^{-3} |

E_{0} |
= | 16.31 | Mev |

K | = | 281.6 | Mev |

K' | = | -286.5 | Mev |

J | = | 36.95 | Mev |

L | = | 110.99 | Mev |

K_{sym} |
= | 33.7 | MeV |

#### Neutron Star Properties

M_{max} |
= | 2.21 | M_{sun} |

MDU,e_{} |
= | 0.9 | M_{sun} |

R_{Mmax} |
= | 12.53 | km |

R_{1.4} |
= | 14.5 | km |

#### References

##### References to the original work:

- [HSNP_2010] M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
- [SHF_2013] A.W. Steiner, M. Hempel, and T. Fischer, Astrophys.J. 774,17 (2013)

##### Further references:

- [HFSLA_2012] M. Hempel, T. Fischer, J. Schaffner-Bielich, and M. LiebendÃ¶rfer, Astrophys. J. 748, 70 (2012)

#### Data sheet

#### Data

eos.zip (1.26 MB) |

eos.zip_checksum.txt |

## Single files |

eos.compo |

eos.init |

eos.micro |

eos.mr |

eos.nb |

eos.t |

eos.thermo |

eos.yq |