The discussion centers on the existence of particles with properties similar to Weakly Interacting Massive Particles (WIMPs) within the Standard Model of Particle Physics. While neutrinos share some characteristics with WIMPs, they do not possess the requisite mass, which is typically in the 100 GeV range. The term WIMP has evolved, and while it can refer to any weakly interacting dark matter candidate, it traditionally denotes particles produced through thermal freeze-out. Various other dark matter candidates are mentioned, including keV sterile neutrinos and supersymmetric particles, but none have been definitively discovered. The complexity of dark matter remains a significant challenge, with ongoing debates about the mass and nature of its constituent particles.