SFH(SFHo) neutron matter (no electrons)
Abstract
This is the zero electron faction EOS table with RMF interactions SFHo [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 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. [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 | = | 1.90e+00 |
| nb pts | = | 308 |
| Y min | = | 0.0 |
| Y max | = | 0.0 |
| Y pts | = | 1 |
Nuclear Matter Properties
| ns | = | 0.1583 | fm-3 |
| E0 | = | 16.19 | Mev |
| K | = | 245.4 | Mev |
| K' | = | -467.8 | Mev |
| J | = | 31.57 | Mev |
| L | = | 47.1 | Mev |
| Ksym | = | -205.4 | MeV |
Neutron Star Properties
| Mmax | = | 2.06 | Msun |
| MDU,e | = | N/A | Msun |
| RMmax | = | 10.32 | km |
| R1.4 | = | 11.9 | 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. Liebendörfer, Astrophys. J. 748, 70 (2012)
Data sheet
Data
| eos.zip (1.19 MB) |
| eos.zip_checksum.txt |
Single files |
| eos.compo |
| eos.init |
| eos.micro |
| eos.mr |
| eos.nb |
| eos.t |
| eos.thermo |
| eos.yq |