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SNSH(TM1e) zero temperature


This table contains the zero temperature version of 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 the website of K. Sumiyoshi (alternatively from the mirror sites or

Nparam = 2
Particles = npeN
T min = 0.0
T max = 0.0
T pts = 1
nb min = 7.59e-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)
[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)
[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)

Data sheet

Data (contains all following files and data sheet)

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

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