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XMLSLZ(GM1)

Abstract

This table corresponds to the unified EoS of neutron star (npeµ) matter at zero temperature and β-equilibrium [XMLSL_2022], which is obtained in the framework of Thomas-Fermi approximation and assuming geometrical symmetries for the Wigner-Seitz cells [XSMLL_2022]. The covariant density functional GM1 is adopted [GMPR_1991].

Nparam = 1
Particles = npemN
T min = 0.0
T max = 0.0
T pts = 1
nb min = 7.59e-11
nb max = 2.00e+00
nb pts = 1078
Y min = 0.0
Y max = 0.0
Y pts = 1

Nuclear Matter Properties

ns = 0.153 fm-3
E0 = 16.33 Mev
K = 300.5 Mev
K' = N/A Mev
J = 32.5 Mev
L = 94.0 Mev
Ksym = 18.0 MeV

Neutron Star Properties

Mmax = 2.36 Msun
MDU,e = 1.28 Msun
RMmax = 11.95 km
R1.4 = 13.76 km

References

References to the original work:
[GMPR_1991]   N. K. Glendenning and S. A. Moszkowski, Phys. Rev. Lett. 67, 2414 (1991)
[XMLSL_2022]   C.-J. Xia, T. Maruyama, A. Li, B. Y. Sun, W.-H. Long, and Y.-X. Zhang, Commun.Theor. Phys. 74, 095303 (2022)
[XSMLL_2022]   C.-J. Xia, B. Y. Sun, T. Maruyama, W.-H. Long, and A. Li, Phys. Rev. C 105, 045803 (2022)

Data sheet

eos.pdf

Data

eos.zip (0.17 MB)
eos.zip_checksum.txt
Single files
eos.t
eos.nb
eos.yq
eos.thermo
eos.compo
eos.init
eos.mr
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