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OPGR(GM1Y5) (with hyperons)

Abstract

This EoS is the classical RMF parameterisation GM1 [GMPR_1991] 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 nB = 10^{−3} fm^{−3}. Hadronic charge 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 = 1.30e+00
nb pts = 347
Y min = 0.0
Y max = 0.0
Y pts = 1

Nuclear Matter Properties

ns = 0.0 fm-3
E0 = 0.0 Mev
K = 0.0 Mev
K' = 0.0 Mev
J = 0.0 Mev
L = 0.0 Mev
Ksym = 0.0 MeV

Neutron Star Properties

Mmax = 0.0 Msun
MDU,e = 0.0 Msun
RMmax = 0.0 km
R1.4 = 0.0 km

References

References to the original work:
[GMPR_1991]   N. K. Glendenning and S. A. Moszkowski, Phys. Rev. Lett. 67, 2414 (1991)
[OPGR_2015]   M. Oertel, C. Providencia, F. Gulminelli, A. Raduta, J. Phys. G 42, 075202 (2015)
[DHA_2001]   F. Douchin, P. Haensel, Astronomy and Astrophysics 380, 151 (2001)

Data sheet

eos.pdf

Data

eos.zip (0.07 MB)
eos.zip_checksum.txt
Single files
eos.compo
eos.init
eos.nb
eos.t
eos.thermo
eos.yq
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