FYSS(TM1) (no electrons)
In the present equation of state, the relativistic mean field theory with the TM1 parameter set for nucleons has been adopted, the quantum approach for d, t, h and alpha, as well as the liquid drop model for the other nuclei under the assumption of nuclear statistical equilibrium. Temperature dependences of surface and shell energies of heavy nuclei have been taken into account as well as the possibility of pasta phases for heavy nuclei and the Pauli- and self-energy shifts for d, t, h and alpha. Further details can be found in Refs.~[ FYSS_2011, FYSS_2013, FYSS_2017 ]. The present version of the table does not include contributions from leptons and photons.
Nuclear Matter Properties
Neutron Star Properties
References to the original work:
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