HS(IUF) neutron matter (no electrons)
Abstract
This is the zero electron fraction EOS table with RMF interactions IUFSU [FHPSP_2010]. 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 electron fraction can be found in Ref. [HSNP_2010], where the TMA interactions were used. The manual from the web page at astro.physik.unibas.ch/ gives further information about the table. Applications of HS EOS for various different RMF interactions in supernova simulations can be found in Refs. [HFSLA_2012,SHF_2013].
| 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
| ns | = | 0.1546 | fm-3 |
| E0 | = | 16.39 | Mev |
| K | = | 231.3 | Mev |
| K' | = | -290.3 | Mev |
| J | = | 31.29 | Mev |
| L | = | 47.2 | Mev |
| Ksym | = | 28.5 | MeV |
Neutron Star Properties
| Mmax | = | 1.95 | Msun |
| MDU,e | = | 1.8 | Msun |
| RMmax | = | 11.31 | km |
| R1.4 | = | 12.7 | km |
References
References to the original work:
- [HSNP_2010] M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
- [FHPSP_2010] F.J. Fattoyev, C.J. Horowitz, J. Piekarewicz, and G. Shen, Phys. Rev. C 82, 055803 (2010)
Further references:
- [HFSLA_2012] M. Hempel, T. Fischer, J. Schaffner-Bielich, and M. Liebendörfer, Astrophys. J. 748, 70 (2012)
- [SHF_2013] A.W. Steiner, M. Hempel, and T. Fischer, Astrophys.J. 774,17 (2013)