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STOS with Lambda hyperons

Abstract

This table contains the EoS of H. Shen, F. Yang, H. Toki, K. Oyamatsu, and K. Sumiyoshi [STOSP_1998,STOSN_1998] with only baryonic contributions (no leptons or photons included) including Lambda hyperons [STOS_2011] 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 was taken from the website user.numazu-ct.ac.jp/ of K. Sumiyoshi.

Nparam = 3
Particles = npaNRBs
T min = 1.00e-01
T max = 3.98e+02
T pts = 92
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

References to the original work:
[STOSP_1998]   H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Prog. Theor. Phys. 100, 1013 (1998)
[SYTP_2006]   H. Shen, F. Yang, H. Toki, Prog. Theor. Phys. 115, 325 (2006)
[STOSN_1998]   H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi, Nucl. Phys. A 637, 435 (1998)
[STOS_2011]   H. Shen, H. Toki, K. Oyamatsu , K. Sumiyoshi, Astrophys.J.Suppl. 197, 20 (2011)
Further references:
[STNP_1994]   Y. Sugahara, H. Toki, Nucl. Phys. A 579, 557 (1994)

Data sheet

Data

eos.zip (contains all following files and data sheet)
eos.compo
eos.init
eos.micro
eos.nb
eos.t
eos.thermo
eos.yq
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The EoS "STOS with Lambda hyperons" has not eos.init file associated so computation is not possible.

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