SFH(SFHo) neutron matter (with electrons)
Abstract
This is the zero electron fraction EOS table with RMF interactions SFHo [SHF_2013]. Contributions of neutrons, anti-neutrons, protons, anti-protons, electrons, positrons, and photons are included, whereas the net abundances of electrons and protons are 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 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 | = | npe 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 (1.28 MB) |
| eos.zip_checksum.txt |
Single files |
| eos.compo |
| eos.init |
| eos.micro |
| eos.mr |
| eos.nb |
| eos.t |
| eos.thermo |
| eos.yq |