DDHdelta model (no hyperons)
Abstract
This EoS is based on the RMF parameterisation DDHdelta [GNPA_2004] for cold neutron star matter in beta-equilibrium containing nucleons and electrons. For the crust, the EoS by Douchin and Haensel [DHA_2001] has been added below a density of nB = 2.5 × 10^{−4} fm^{−3} and the inner crust has been computed following [GPPVP_2014]. Proton fraction and compositional information is available for the core only.
| Nparam | = | 1 |
| Particles | = | npe |
| T min | = | 0.0 |
| T max | = | 0.0 |
| T pts | = | 1 |
| nb min | = | 7.93e-15 |
| nb max | = | 1.00e+00 |
| nb pts | = | 428 |
| Y min | = | 0.0 |
| Y max | = | 0.0 |
| Y pts | = | 1 |
Nuclear Matter Properties
| ns | = | 0.0 | fm-3 |
| E0 | = | 0.0 | Mev |
| K | = | 0.0 | Mev |
| K' | = | 0.0 | Mev |
| J | = | 0.0 | Mev |
| L | = | 0.0 | Mev |
| Ksym | = | 0.0 | MeV |
Neutron Star Properties
| Mmax | = | 0.0 | Msun |
| MDU,e | = | 0.0 | Msun |
| RMmax | = | 0.0 | km |
| R1.4 | = | 0.0 | km |
References
References to the original work:
- [GNPA_2004] T. Gaitanos et al., Nucl. Phys. A732, 24 (2004)
- [GPPVP_2014] F. Grill, H. Pais, C. Providencia, I. Vidana and S. S. Avancini, Phys. Rev. C 90, 045803 (2014)
- [DHA_2001] F. Douchin, P. Haensel, Astronomy and Astrophysics 380, 151 (2001)