HS(FSG) neutron matter (no electrons)
Abstract
This is the zero electron fraction EOS table with RMF interactions FSUgold [TPPR_2005]. 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 https://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 | = | 0.1482 | fm-3 |
| E0 | = | 16.27 | Mev |
| K | = | 229.5 | Mev |
| K' | = | -523.9 | Mev |
| J | = | 32.56 | Mev |
| L | = | 60.43 | Mev |
| Ksym | = | -51.4 | MeV |
Neutron Star Properties
| Mmax | = | 1.74 | Msun |
| MDU,e | = | 1.4 | Msun |
| RMmax | = | 10.95 | km |
| R1.4 | = | 12.6 | km |
References
References to the original work:
- [HSNP_2010] M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
- [TPPR_2005] B.G. Todd-Rutel and J. Piekarewicz, Phys. Rev. Lett. 95 , 122501 (2005)
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)
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 |