  Using the nuclear equation of states for a large variety of relativistic and
non-relativistic force parameters, we calculate the static and rotating masses
and radii of neutron stars. From these equation of states, we also evaluate the
properties of rotating neutron stars, such as rotational and gravitational
frequencies, moment of inertia, quadrupole deformation parameter, rotational
ellipcity and gravitational wave strain amplitude. The estimated gravitational
wave strain amplitude of the star is found to be $\sim 10^{-23}$.
