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HS_NL3 neutron matter (with electrons)


This is the zero electron faction EOS table with RMF interactions NL3 [LKRP_1997]. 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 Y e 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 = 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:
[HSNP_2010]   M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
[LKRP_1997]   G.A. Lalazissis, J. K├Ânig, and P. Ring, Phys. Rev. C 55, 540 (1997)
Further references:
[HFSLA_2012]   M. Hempel, T. Fischer, J. Schaffner-Bielich, and M. Liebend├Ârfer, 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_NL3 neutron matter (with electrons)" has not eos.init file associated so computation is not possible.

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