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HS_IUF neutron matter (no electrons)


This is the zero electron fraction EOS table with RMF interactions IUFSU [FHPSP_2010]. 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], where the TMA interactions were used. The manual from the web page at 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 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)
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_IUF neutron matter (no electrons)" has not eos.init file associated so computation is not possible.

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