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HS_TMA neutron matter (no electrons)

Abstract

This is the zero electron fraction EOS table with RMF interactions TMA [THSSN_1995]. Contributions of neutrons, anti-neutrons, protons, and anti-protons are included, whereas the net abundance of protons is always zero. The details of the underlying EOS model at finite electron fraction can be found in Ref. [HSNP_2010]. The manual from the web page at astro.physik.unibas.ch 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 = np 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

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

eos.zip (contains all following files and data sheet)
eos.compo
eos.init
eos.micro
eos.mr
eos.nb
eos.t
eos.thermo
eos.yq
Compute
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The EoS "HS_TMA neutron matter (no electrons)" has not eos.init file associated so computation is not possible.

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