TSO(DDLS(50)-N)
Abstract
This general-purpose hadronic EoS table, based on the work of Ref. [TSO_2024 ], is generated by following the covariant density functional (CDF) approach. The high-density phase consists of npe matter, in which the coupling constants of the baryons are density- dependent (DD), selected appropriately so that the slope of the symmetry energy is Lsym = 50 MeV and the skewness equals Qsat = 400 MeV, using the DDLS family of parametrizations [ LS_2023 ]. The extension to lower densities was done by matching to the low- density HS(DD2) model [HSNP_2010 ], which is developed through an improved nuclear statistical equilibrium among nucleons and nuclear clusters.
| Nparam | = | 3 |
| Particles | = | npe |
| T min | = | 1.00e-01 |
| T max | = | 1.58e+02 |
| T pts | = | 81 |
| nb min | = | 1.00e-12 |
| nb max | = | 1.20e+00 |
| nb pts | = | 303 |
| Y min | = | 1.00e-02 |
| Y max | = | 6.00e-01 |
| Y pts | = | 60 |
Nuclear Matter Properties
| ns | = | 0.152 | fm-3 |
| E0 | = | 16.14 | Mev |
| K | = | 251.0 | Mev |
| K' | = | 400.0 | Mev |
| J | = | 32.2 | Mev |
| L | = | 50.0 | Mev |
| Ksym | = | N/A | MeV |
Neutron Star Properties
| Mmax | = | 2.47 | Msun |
| MDU,e | = | N/A | Msun |
| RMmax | = | 12.16 | km |
| R1.4 | = | 13.15 | km |