OPGR(DDHdeltaY4) (with hyperons)
Abstract
This EoS is based on the RMF parameterisation DDHdelta~[GNPA_2004] for cold neutron star matter in beta-equilibrium containing the baryon octet and electrons, see Ref.~[OPGR_2015] for details of the parameterisation of hyperonic interactions. For the crust, the EoS by Douchin and Haensel [DHA_2001] has been added below a density of n_B = 2.5 x 10^(-4) fm^(-3) and the inner crust has been computed following~[GPPVP_2014]. Proton fraction and compositional information is available for the core only.
Nparam | = | 1 |
Particles | = | npeBs |
T min | = | 0.0 |
T max | = | 0.0 |
T pts | = | 1 |
nb min | = | 7.93e-15 |
nb max | = | 9.86e-01 |
nb pts | = | 307 |
Y min | = | 0.0 |
Y max | = | 0.0 |
Y pts | = | 1 |
Nuclear Matter Properties
ns | = | 0.153 | fm-3 |
E0 | = | 16.3 | Mev |
K | = | 240.0 | Mev |
K' | = | N/A | Mev |
J | = | 25.1 | Mev |
L | = | 44.0 | Mev |
Ksym | = | N/A | MeV |
Neutron Star Properties
Mmax | = | 2.05 | Msun |
MDU,e | = | N/A | Msun |
RMmax | = | 11.26 | km |
R1.4 | = | 12.58 | km |
References
References to the original work:
- [GNPA_2004] T. Gaitanos et al., Nucl. Phys. A732, 24 (2004)
- [OPGR_2015] M. Oertel, C. Providencia, F. Gulminelli, A. Raduta, J. Phys. G 42, 075202 (2015)
- [GPPVP_2014] F. Grill, H. Pais, C. Providencia, I. Vidana and S. S. Avancini, Phys. Rev. C 90, 045803 (2014)
- [DHA_2001] F. Douchin, P. Haensel, Astronomy and Astrophysics 380, 151 (2001)
Data sheet
Data
eos.zip (0.06 MB) |
eos.zip_checksum.txt |
Single files |
eos.compo |
eos.init |
eos.nb |
eos.t |
eos.thermo |
eos.yq |