GPPVA(FSU2) NS unified inner crust-core
Abstract
This inner crust-core unified EoS for beta-equilibrium matter at zero temperature is con- structed with a BPS outer crust [BPSA_1971] below baryon density of 0.002 fm^{−3}., an inner crust EoS [PFPR_2019], including nonspherical pasta phases, calculated within a self-consistent Thomas-Fermi approach [GPPVP_2014], and a homogeneous npe\mu core EoS, above baryon density of 0.054 fm^{−3}. The EoS parameterisation used was the non-linear RMF FSU2 model [CP_2014].
Nparam | = | 1 |
Particles | = | None |
T min | = | 0.0 |
T max | = | 0.0 |
T pts | = | 1 |
nb min | = | 6.30e-12 |
nb max | = | 2.10e+00 |
nb pts | = | 253 |
Y min | = | 0.0 |
Y max | = | 0.0 |
Y pts | = | 1 |
Nuclear Matter Properties
ns | = | 0.1505 | fm-3 |
E0 | = | -16.28 | Mev |
K | = | 238.0 | Mev |
K' | = | -149.0 | Mev |
J | = | 37.6 | Mev |
L | = | 113.0 | Mev |
Ksym | = | 25.0 | MeV |
Neutron Star Properties
Mmax | = | 2.07 | Msun |
MDU,e | = | 0.0 | Msun |
RMmax | = | 12.08 | km |
R1.4 | = | 13.89 | km |
References
References to the original work:
- [GPPVP_2014] F. Grill, H. Pais, C. Providencia, I. Vidana and S. S. Avancini, Phys. Rev. C 90, 045803 (2014)
- [BPSA_1971] G. Baym, C. Pethick and P. Sutherland, Astrophys. J. 170, 299 (1971)
- [PFPR_2019] C. Providência, M. Fortin, H. Pais, and A. Rabhi, Astron. Space Sci. 6, 13 (2019)
- [CP_2014] W.-C. Chen and J. Piekarewicz, Phys. Rev. C 90, 044305 (2014)
Data sheet
Data
eos.zip (0.13 MB) |
eos.zip_checksum.txt |
Single files |
eos.init |
eos.nb |
eos.t |
eos.yq |
eos.thermo |
eos.mr |