References for the supernova EOS tables

The original HS EOS model was published in the Nucl. Phys. A article listed below. In this article the TMA interactions were used and the corresponding EOS was discussed in great detail. The SFHo and SFHx tables also have their own reference and the BHBΛ and BHBΛφ tables as well. The tables for TM1 and FSUgold have been applied in core-collapse supernova simulations in the articles from Steiner et al. and Hempel et al., where their properties are at least briefly discussed. Therefore these two articles can be used as references for the TM1 and FSUgold tables. The properties of all of the eight EOS tables are briefly discussed and compared with each other in the article from Fischer et al. In this article, DD2 has been used for the first time in core-collapse supernova simulations.

The article from Hempel 2014 discusses nucleon single-particle properties such as the self-energies or effective masses of the same EOS tables. In addition, simple expressions for consistent weak charged-current rates are given.

For all tables, especially for the unpublished ones, additionally something like the following sentence can be used as a reference/specification:

"We apply the supernova EOS table calculated with the model of Hempel & Schaffner-Bielich (2010), whereas the XX nucleon interactions [XX] and the nuclear mass table from Ref. [YY] have been used [M. Hempel, private communication]."

For 'XX' the correct name and reference of the RMF parameterization of the nucleon interactions should be chosen, and for 'YY' the correct reference to the mass model. Please write me if you have any questions. 

• Hempel, M.
  Nucleon self-energies and weak charged-current rates for existing relativistic supernova equations of state
  arXiv:1410.6337
  NASA ADS URL


• Banik, S.; Hempel, M.; Bandyophadyay, D.
  New hyperon equations of state for supernovae and neutron stars in density dependent hadron field theory
  Astrophys. J. Suppl. 214, 22 (2014)
  NASA ADS URL

• Fischer, T.; Hempel, M.; Sagert, I.; Suwa, Y.; Schaffner-Bielich, J.
  Symmetry energy impact in simulations of core-collapse supernovae
  Eur. Phys. J. A 50, 46 (2014)
  NASA ADS URL


• Steiner, A.; Hempel, M.; Fischer, T.
  Core-collapse supernova equations of state based on neutron star observations
  Astrophys. J. 774, 17 (2013)
  NASA ADS URL


• Hempel, M.; Fischer T.; Schaffner-Bielich, J.; Liebendörfer M.
  New equations of state in core-collapse supernova simulations
  Astrophys. J. 748, 70 (2012)
  NASA ADS URL


• Hempel, M.; Schaffner-Bielich, J.
  A Statistical Model for a Complete Supernova Equation of State
  Nucl. Phys. A 837, 210-254 (2010)
  NASA ADS URL

• TMA
  Toki et al., Nucl. Phys. A 588, 357 (1995)
  NASA ADS URL
  
  
• TM1
  Sugahara and Toki, Nucl. Phys. A 579, 557 (1994)
  NASA ADS URL
  
  
• FSUgold
  Todd-Rutel and Piekarewicz, Phys. Rev. L. 95, 122501 (2005)
  NASA ADS URL
  
  
• NL3
  Lalazissis et al., Phys. Rev. C 55, 540 (1997)
  NASA ADS URL
  
  
• DD2
  Typel et al., Phys. Rev. C 81, 015803 (2010)
  NASA ADS URL
  
  
• SFHo and SFHx
  Steiner et al., Astrophys. J. 774, 17 (2013)
  NASA ADS URL
  
  
• IUFSU
  Fattoyev et al., Phys. Rev. C82, 055803 (2010)
  NASA ADS URL

• AWT
  Audi et al., Nucl. Phys. A 729, 337 (2003)
  NASA ADS URL

• FRDM
  Möller et al, ADNDT 59, 185 (1995)
  NASA ADS URL
  
  

• TMA
  Geng et al., Prog. Theor. Phys. 113, 785 (2005)
  NASA ADS URL
  
  

• FSUgold
  X. Roca-Maza, private communication, see also Roca-Maza and Piekarewicz, Phys. Rev. C 78, 025807 (2008) 
  NASA ADS URL
  
  

• NL3
  Lalazissis et al., ADNDT 71, 1 (1999) 
  NASA ADS URL