GPPVA(FSU2H) NS unified inner crust-core
Abstract
This inner crust-core unified EoS for beta-equilibrium matter at zero temperature is constructed 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 densit of 0.087 fm^{-3}. The EoS parameterisation used was the non-linear RMF FSU2H model [ NTCRD_2018].
Nparam | = | 1 |
Particles | = | None |
T min | = | 0.0 |
T max | = | 0.0 |
T pts | = | 1 |
nb min | = | 6.30e-12 |
nb max | = | 3.38e+00 |
nb pts | = | 282 |
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' | = | -24.6 | Mev |
J | = | 30.5 | Mev |
L | = | 44.5 | Mev |
Ksym | = | 87.0 | MeV |
Neutron Star Properties
Mmax | = | 2.37 | Msun |
MDU,e | = | 0.0 | Msun |
RMmax | = | 12.43 | km |
R1.4 | = | 13.29 | 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)
- [NTCRD_2018] R. Negreiros, L. Tolos, M. Centelles, A. Ramos, and V. Dexheimer, Astrophys. J. 863, 104 (2018)
- [PFPR_2019] C. Providência, M. Fortin, H. Pais, and A. Rabhi, Astron. Space Sci. 6, 13 (2019)
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 |