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This table contains the EoS of H. Shen, F. Ji, J. Hu and K. Sumiyoshi [SJHS_2030 ,SNSHS_2019 ] using a non-linear relativistic mean-field model with the TM1e parametrization [BHZS_2014 ] of the effective interaction. Compared with the original version [STOSN_1998 ,STOSP_1998 ] using the TM1 parametrization [STNP_1994], a density dependent symmetry energy has been introduced [BHZS_2014]. 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 was taken from thewebsite of K. Sumiyoshi (alternatively from the mirror sites or The contribution of electrons and photons has been added to the original table.

Nparam = 3
Particles = npeN
T min = 1.00e-01
T max = 3.98e+02
T pts = 91
nb min = 7.60e-11
nb max = 6.02e+00
nb pts = 110
Y min = 1.00e-02
Y max = 6.50e-01
Y pts = 65


References to the original work:
[SNSHS_2019]   K. Sumiyoshi, K. Nakazato, H. Suzuki, J. Hu, H. Shen, Astrophys. J 887, 110 (2019)
[STNP_1994]   Y. Sugahara, H. Toki, Nucl. Phys. A 579, 557 (1994)
[STOSN_1998]   H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Nucl. Phys. A 637, 435 (1998)
[STOSP_1998]   H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Prog. Theor. Phys. 100, 1013 (1998)
[BHZS_2014]   S. S. Bao, J. N. Hu, Z. W. Zhang, and H. Shen, Phys. Rev. C 90, 045802 (2014)
[SJHS_2020]   H. Shen, F. Ji, J. Hu, K. Sumiyoshi, arXiv:2001.10143 (2020)

Data sheet

Data (contains all following files and data sheet)

The EoS "SNSH(TM1e)" has not eos.init file associated so computation is not possible.

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