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  Relativistic EOS for core-collapse SN simulations (Shen+, 2011)
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1.J/ApJS/197/20/eos2EOS2 model of core-collapse SN simulation [model](tables 3, 4 and 5 of paper) (Note) (667920 rows)

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ShowSortColumn  Constraint Explain   (UCD)
  T MeV [0/400] Temperature (phys.temperature)
  logpB [g/cm3] [5.1/16] Log of baryon mass density (phys.density)
  nB fm-3 Baryon number density (;meta.main)
  Yp   [0/1] Proton fraction (meta.number)
  isoT  Plot this isotherm (meta.ref.url)
  isod  Plot this iso-density (meta.ref.url)
  F MeV Free energy per baryon (Note G1)   (
  Eint MeV Internal energy per baryon (Note G2)   (
  S/k  Entropy per baryon (in units of Boltzmann's k) (
  A  Mass number of heavy nucleus (phys.atmol.weight)
  Z  Charge number of heavy nucleus (phys.atmol.number)
  M*N MeV Effective nucleon mass (phys.mass)
  Xn   [0/1] Free neutron fraction (phys.abund)
  Xp   [0/1] Free proton fraction (phys.abund)
  Xa   [0/1] α-particle fraction (phys.abund)
  XA   [0/1] heavy nucleus fraction (phys.abund)
  P MeV/fm3 Pressure (phys.pressure)
  mun MeV Chemical potential of the neutron (Note G3)   (;phys.atmol.level)
  mup MeV Chemical potential of the proton (Note G3)   (;phys.atmol.level)

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