[en] The properties of massive neutron stars and protoneutron stars are studied in this work in the framework of relativistic mean-field theory. For certain choices of coupling parameters, a two-solar mass cold neutron star is obtained in the presence of hyperons, taking into account the influence of ${\mathrm{\sigma <!--\; ??\; -->}}^{\ast <!--\; ???\; -->}$ and ϕ mesons. The model for the coupling parameters is then extrapolated to study the effects of ${\mathrm{\sigma <!--\; ??\; -->}}^{\ast <!--\; ???\; -->}$ and ϕ mesons on the properties of massive protoneutron stars in different evolutionary stages. The coupling constants are determined by two different methods, and their corresponding influence on the equation of state, mass, radius, and temperature is studied. The effect of the strange mesons is different at different evolution stages of the neutron star. The properties of a protoneutron star corresponding to the mass of PSR J0348+0432 are also presented.