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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

eos.pdf

Data

eos.zip (0.13 MB)
eos.zip_checksum.txt
Single files
eos.init
eos.nb
eos.t
eos.yq
eos.thermo
eos.mr
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