HS(DD2) (no electrons)
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 DD2 [TRKBP_2010]. Contributions of neutrons, anti-neutrons, protons, anti-protons, and nuclei are in- cluded. For the masses of nuclei, FRDM [MNKA_1997] was used. 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 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].
Nuclear Matter Properties
Neutron Star Properties
References to the original work:
- [HSNP_2010] M. Hempel and J. Schaffner-Bielich, Nucl. Phys. A 837, 210 (2010)
- [TRKBP_2010] S. Typel, G. Röpke, T. Klähn, D. Blaschke, and H.H. Wolter, Phys. Rev. C 81, 015803 (2010)
- [MNKA_1997] P. Möller, J.R. Nix, and K.-L. Kratz, Atomic Data and Nuclear Data Tables 66, 131 (1997)