GMSR(H1)
Abstract
This table corresponds to the unified EoS of cold catalized nuclear matter at β-equilibrium by G. Grams, J. Margueron, R. Somosundaram and S. Reddy [GMSR_2021]. The crust is model with a compressible liquid drop model (CLDM) with Coulomb, surface and curvature terms, the crust model is named finite size 4 (FS4). The considered effective interaction is given by the non-relativistic (NR) meta-model (MM) adjusted to reproduce the Chiral EFT Hamilatonian H1. The lowest order nuclear empirical parameters (E, L / n, K ) are defined from a fit of symmetric matter (SM) and neutron matter (NM) to the original model, while the higher order ones (K', Z) are fixed to reach a 2Msun neutron star. See Ref. [GMSR_2021].
| Nparam | = | 1 |
| Particles | = | npemN |
| T min | = | 0.0 |
| T max | = | 0.0 |
| T pts | = | 1 |
| nb min | = | 1.00e-07 |
| nb max | = | 2.00e+00 |
| nb pts | = | 485 |
| Y min | = | 0.0 |
| Y max | = | 0.0 |
| Y pts | = | 1 |
Nuclear Matter Properties
| ns | = | 0.186 | fm-3 |
| E0 | = | -17.0 | Mev |
| K | = | 261.0 | Mev |
| K' | = | 220.0 | Mev |
| J | = | 33.8 | Mev |
| L | = | 46.8 | Mev |
| Ksym | = | -154.0 | MeV |
Neutron Star Properties
| Mmax | = | 2.28 | Msun |
| MDU,e | = | N/A | Msun |
| RMmax | = | 10.53 | km |
| R1.4 | = | 11.58 | km |
References
References to the original work:
- [GMSR_2021] G. Grams, J. Margueron, R. Somasundaram and S. Reddy, Eur.Phys.J.A 58 (2022) 56 (2022)
Data sheet
Data
| eos.zip (0.16 MB) |
| eos.zip_checksum.txt |
Single files |
| eos.mr |
| eos.compo |
| eos.init |
| eos.nb |
| eos.t |
| eos.thermo |
| eos.yq |