Dark matter is theorized to exist primarily to explain the gravitational binding of galaxies, yet no direct evidence of its clumping has been found, which is necessary for it to bend light. While dark matter is essential for cosmological models, such as the WMAP data on cosmic microwave background anisotropies, it remains undetected in laboratory experiments. Gravitational lensing, where light from distant quasars is bent by the gravitational influence of nearby galaxies, suggests dark matter's presence in massive halos around these galaxies. The standard Lambda Cold Dark Matter (LCDM) model posits that dark matter constitutes about 27% of the universe's density, with only 4% being ordinary matter. Despite its theoretical importance, the exact nature of dark matter remains elusive and continues to be a significant topic in astrophysics.