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HS_TMA neutron matter (with electrons)


This is the zero electron fraction EOS table with RMF interactions TMA [THSSN_1995]. Contributions of neutrons, anti-neutrons, protons, anti-protons, electrons, positrons, and photons are included, whereas the net abundances of electrons and protons are always zero. The details of the underlying EOS model at finite electron fraction can be found in Ref. [HSNP_2010]. The manual from this web page gives further information about the table. Applications of HS EOS for various different RMF interactions in supernova simulations can be found in Refs. [HFSLA_2012,SHF_2013].

Nparam = 2
Particles = npe N
T min = 1.00e-01
T max = 1.58e+02
T pts = 81
nb min = 1.00e-12
nb max = 1.00e+01
nb pts = 326
Y min = 0.0
Y max = 0.0
Y pts = 1


References to the original work:
[THSSN_1995]   H. Toki, D. Hirata, Y. Sugahara, K. Sumiyoshi, and I. Tanihata, Nucl. Phys. A 588, 357 (1995)
[HSNP_2010]   M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
Further references:
[HFSLA_2012]   M. Hempel, T. Fischer, J. Schaffner-Bielich, and M. Liebendörfer, Astrophys. J. 748, 70 (2012)
[SHF_2013]   A.W. Steiner, M. Hempel, and T. Fischer, Astrophys.J. 774,17 (2013)

Data sheet

Data (contains all following files and data sheet)

The EoS "HS_TMA neutron matter (with electrons)" has not eos.init file associated so computation is not possible.

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