RG(SLY4)
Abstract
This table corresponds to the zero temperature and beta-equilibrium unified EoS by Gulminelli and Raduta [GR_2015]. The considered effective interaction is SLy4 [CBHMS_1998]. Cluster energy functionals are those of Ref. [DLNP_2009].
Nparam | = | 1 |
Particles | = | npemN |
T min | = | 0.0 |
T max | = | 0.0 |
T pts | = | 1 |
nb min | = | 1.00e-07 |
nb max | = | 1.21e+00 |
nb pts | = | 197 |
Y min | = | 0.0 |
Y max | = | 0.0 |
Y pts | = | 1 |
Nuclear Matter Properties
ns | = | 0.159 | fm-3 |
E0 | = | 15.97 | Mev |
K | = | 230.0 | Mev |
K' | = | -363.11 | Mev |
J | = | 32.04 | Mev |
L | = | 46.0 | Mev |
Ksym | = | -119.73 | MeV |
Neutron Star Properties
Mmax | = | 2.06 | Msun |
MDU,e | = | N/A | Msun |
RMmax | = | 10.02 | km |
R1.4 | = | 11.7 | km |
References
References to the original work:
- [DLNP_2009] P. Danielewicz et J. Lee, Nucl. Phys. A818, 36 (2009)
- [GR_2015] F. Gulminelli and Ad. R. Raduta, Phys. Rev. C 92, 055803 (2015)
- [CBHMS_1998] E. Chabanat, P. Bonche, P. Haensel, J. Meyer, and R. Schaeffer, Nucl. Phys. A 635, 231 (1998)
Data sheet
Data
eos.zip (0.12 MB) |
eos.zip_checksum.txt |
Single files |
eos.compo |
eos.init |
eos.mr |
eos.nb |
eos.t |
eos.thermo |
eos.yq |