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STOS(TM1) (original version)

Abstract

This table contains the EoS of H. Shen, H. Toki, K. Oyamatsu, and K. Sumiyoshi [STOSP_1998,STOSN_1998] with only baryonic contributions (no leptons or photons included) using a non-linear relativistic mean-field model with the TM1 parametrization [STNP_1994] of the effective interaction. Non-uniform nuclear matter is calculated in the single-nucleus Thomas-Fermi approximation with parametrized density distributions in spherical Wigner-Seitz cells. Only neutrons, protons, alpha particles and a single heavy nucleus are considered. The present table is the original version that was taken from the website user.numazu-ct.ac.jp/ of K. Sumiyoshi. An update with higher resolution (new version) is available in the CompOSE database.

Nparam = 3
Particles = npaNR
T min = 1.00e-01
T max = 1.00e+02
T pts = 31
nb min = 7.59e-11
nb max = 1.73e+00
nb pts = 104
Y min = 1.00e-02
Y max = 5.62e-01
Y pts = 71

Nuclear Matter Properties

ns = 0.145 fm-3
E0 = 16.26 Mev
K = 281.16 Mev
K' = -285.22 Mev
J = 36.89 Mev
L = 110.79 Mev
Ksym = 33.62 MeV

Neutron Star Properties

Mmax = N/A Msun
MDU,e = N/A Msun
RMmax = N/A km
R1.4 = N/A km

References

References to the original work:
[STOSP_1998]   H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Prog. Theor. Phys. 100, 1013 (1998)
[STOSN_1998]   H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Nucl. Phys. A 637, 435 (1998)
Further references:
[STNP_1994]   Y. Sugahara, H. Toki, Nucl. Phys. A 579, 557 (1994)

Data sheet

eos.pdf

Data

eos.zip (16.86 MB)
eos.zip_checksum.txt
Single files
eos.compo
eos.init
eos.micro
eos.nb
eos.t
eos.thermo
eos.yq
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