Gravity waves are disturbances in the gravitational field, but detecting them through matter-antimatter collisions is challenging due to low energy levels that fail to produce significant effects. Existing experiments have yielded minimal gravitational data from such collisions. In contrast, merging black holes are a strong predicted source of gravitational waves, necessitating large detection apparatus like LIGO and LISA. The difficulty in producing detectable gravitational waves stems from momentum conservation, as oscillating a complete system's center of mass is not feasible like it is with electromagnetic waves. Overall, the detection of gravitational waves remains a complex endeavor requiring substantial energy and advanced technology.