## STOS neutron and Lambda matter

#### Abstract

This table contains the neutron-matter EoS of H. Shen, F. Yang, H. Toki, K. Oyamatsu, and K. Sumiyoshi [STOSP_1998,STOSN_1998] with only baryonic contributions (no leptons or photons included) including Lambda hyperons [STOS_2011] using a non-linear relativistic mean-field model with the TM1 parametrization [STNP_1994] of the effective interaction. Non-uniform nuclear matter is calculated in the single-nucleus Thomas-Fermi approximation with parametrized density distributions in spherical Wigner-Seitz cells. Only neutrons, protons,alpha particles and a single heavy nucleus are considered. The present table was taken from the website user.numazu-ct.ac.jp/ of K. Sumiyoshi.

Nparam | = | 2 |

Particles | = | npBs |

T min | = | 0.0 |

T max | = | 3.98e+02 |

T pts | = | 92 |

nb min | = | 7.59e-11 |

nb max | = | 6.02e+00 |

nb pts | = | 110 |

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

##### References to the original work:

- [STOSP_1998] H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Prog. Theor. Phys. 100, 1013 (1998)
- [SYTP_2006] H. Shen, F. Yang, H. Toki, Prog. Theor. Phys. 115, 325 (2006)
- [STOSN_1998] H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Nucl. Phys. A 637, 435 (1998)
- [STOS_2011] H. Shen, H. Toki, K. Oyamatsu , K. Sumiyoshi, Astrophys.J.Suppl. 197, 20 (2011)

##### Further references:

- [STNP_1994] Y. Sugahara, H. Toki, Nucl. Phys. A 579, 557 (1994)