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HS_IUF (no electrons)

Abstract

This hadronic EOS table is calculated with the statistical model with excluded volume and interactions of Hempel and Schaffner-Bielich (HS) [HSNP_2010] with RMF interactions IUFSU[FHPSP_2010]. Contributions of neutrons, anti-neutrons, protons, anti-protons, and nuclei are included. For the masses of nuclei, an unpublished table generated by X. Roca-Maza was used, see e.g. Ref. [RPPR_2008]. The details of the underlying EOS model can be found in Ref. [HSNP_2010], where the TMA interactions were used. The manual from Matthias Hempel's web page gives further information about the EOS table. On this web page, also routines are available which allow to determine the abundances of all nuclei for all conditions. Applications of HS EOS for various different RMF interactions in supernova simulations can be found in Refs. [HFSLA_2012,SHF_2013].

Nparam = 3
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 = 1.00e-02
Y max = 6.00e-01
Y pts = 60

References

References to the original work:
[HSNP_2010]   M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
[FHPSP_2010]   F.J. Fattoyev, C.J. Horowitz, J. Piekarewicz, and G. Shen, Phys. Rev. C 82, 055803 (2010)
[RPPR_2008]   X. Roca-Maza and J. Piekarewicz, Phys. Rev. C 78, 025807 (2008)
Further references:
[HFSLA_2012]   M. Hempel, T. Fischer, J. Schaffner-Bielich, and M. Liebend√∂rfer, 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_IUF (no electrons)" has not eos.init file associated so computation is not possible.

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