STOS(TM1) (new version) with electrons
This table contains the EoS of H. Shen, H. Toki, K. Oyamatsu, and K. Sumiyoshi [STOSP_1998,STOSN_1998] with only baryonic contributions (no leptons or photons included) using a non-linear relativistic mean-field model with the TM1 parametrization [STNP_1994] of the effective interaction. Non-uniform nuclear matter is calculated in the single-nucleus Thomas-Fermi approximation with parametrized density distributions in spherical Wigner-Seitz cells. Only neutrons, protons, alpha particles and a single heavy nucleus are considered. The present table is the updated high-resolution version that was taken from the website user.numazu-ct.ac.jp/ of K. Sumiyoshi. The contributions from electrons/positrons and photons have been added to the original table.
Nuclear Matter Properties
Neutron Star Properties