Gravitational waves (GWs) predicted by Albert Einstein in 1915. Attempts to detect the gravitational waves go back to the year 1966 during which Max Weber and his colleagues attempted to set up an experiment to detect GWs.ut despite all these efforts,, GWs were first discovered by the Ligo detector in 2016, which resulted in the Nobel Prize being awarded to Rainer Weiss, Barry C. Barish, and Kip S.Thorne. This detector works based on the Michelson interferometer, which has optical Fabry-Perot cavities in its arms. The discovery of gravitational waves has opened a new window on cosmology and astrophysics. In this thesis, we studied the possibility of the generation of polarized GWs. Using the gravitational Stokes parameters, we parameterized the polarization of GWs.We calculated the stokes parameters for GWs emitted from a binary system. We found that the circular polarization of GWs can be generated that is dependent on the GWs line of sight.
