  We construct a complete equation of state (EOS) covering a wide range of
temperature, proton fraction, and baryon density for the use of astrophysical
simulations. We employ the relativistic mean-field (RMF) theory to describe
nuclear interactions and adopt the Thomas-Fermi approximation to describe the
nonuniform nuclear matter. The uniform matter and nonuniform matter are studied
consistently using the same RMF theory.
