  We investigate the effects of meson-mass reduction on the properties of the
neutron star matter. We adopt the Brown-Rho scaling law to take into account
density dependence of meson masses in the quantum hadrodynamics, quark-meson
coupling and modified quark-meson coupling models. It is found that the
equation of state becomes stiff when the mass of meson is reduced in dense
medium. We discuss its implication on the properties of the neutron star.
