HS(NL3) neutron matter (with electrons)
Abstract
This is the zero electron faction EOS table with RMF interactions NL3 [LKRP_1997]. 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 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. [HFSLA_2012,SHF_2013]
| 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 | = | 1.00e+01 |
| nb pts | = | 326 |
| Y min | = | 0.0 |
| Y max | = | 0.0 |
| Y pts | = | 1 |
Nuclear Matter Properties
| ns | = | 0.1482 | fm-3 |
| E0 | = | 16.24 | Mev |
| K | = | 271.5 | Mev |
| K' | = | 202.6 | Mev |
| J | = | 37.39 | Mev |
| L | = | 118.49 | Mev |
| Ksym | = | 100.8 | MeV |
Neutron Star Properties
| Mmax | = | 2.79 | Msun |
| MDU,e | = | 0.9 | Msun |
| RMmax | = | 13.4 | km |
| R1.4 | = | 14.8 | km |
References
References to the original work:
- [HSNP_2010] M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
- [LKRP_1997] G.A. Lalazissis, J. König, and P. Ring, Phys. Rev. C 55, 540 (1997)
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)