HS_FSG neutron matter (no electrons)
This is the zero electron fraction EOS table with RMF interactions FSUgold [TPPR_2005]. 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 https://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].
References to the original work:
- [HSNP_2010] M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
- [TPPR_2005] B.G. Todd-Rutel and J. Piekarewicz, Phys. Rev. Lett. 95 , 122501 (2005)