XMLSLZ(TW99)
Abstract
This table corresponds to the unified EoS of neutron star (npeµ) matter at zero temperature and β-equilibrium [XMLSL_2022], which is obtained in the framework of Thomas-Fermi approximation and assuming geometrical symmetries for the Wigner-Seitz cells [XSMLL_2022]. The covariant density functional TW99 is adopted [TW_1999].
Nparam | = | 1 |
Particles | = | npemN |
T min | = | 0.0 |
T max | = | 0.0 |
T pts | = | 1 |
nb min | = | 7.59e-11 |
nb max | = | 2.00e+00 |
nb pts | = | 1078 |
Y min | = | 0.0 |
Y max | = | 0.0 |
Y pts | = | 1 |
Nuclear Matter Properties
ns | = | 0.153 | fm-3 |
E0 | = | 16.24 | Mev |
K | = | 240.2 | Mev |
K' | = | N/A | Mev |
J | = | 32.8 | Mev |
L | = | 55.3 | Mev |
Ksym | = | N/A | MeV |
Neutron Star Properties
Mmax | = | 2.08 | Msun |
MDU,e | = | N/A | Msun |
RMmax | = | 10.62 | km |
R1.4 | = | 12.27 | km |
References
References to the original work:
- [TW_1999] Typel, S. and Wolter, H.H., Nucl. Phys. A656 ,331 (1999)
- [XMLSL_2022] C.-J. Xia, T. Maruyama, A. Li, B. Y. Sun, W.-H. Long, and Y.-X. Zhang, Commun.Theor. Phys. 74, 095303 (2022)
- [XSMLL_2022] C.-J. Xia, B. Y. Sun, T. Maruyama, W.-H. Long, and A. Li, Phys. Rev. C 105, 045803 (2022)
Data sheet
Data
eos.zip (0.17 MB) |
eos.zip_checksum.txt |
Single files |
eos.t |
eos.nb |
eos.yq |
eos.thermo |
eos.compo |
eos.init |
eos.mr |