The nature of dark matter and dark energy is one of the most significant and enigmatic questions in modern astrophysics and cosmology. These mysterious components make up the majority of the universe’s mass-energy content but are not composed of ordinary matter or energy that we can observe directly. Dark matter is hypothesized to be a form of matter that does not emit, absorb, or interact with electromagnetic radiation (such as light), making it invisible to traditional telescopes. It is inferred to exist based on its gravitational effects on visible matter, such as galaxies and galaxy clusters. Dark energy, on the other hand, is a mysterious force that is driving the accelerated expansion of the universe. Its nature is not well understood, and it appears to be a form of energy associated with empty space itself. The quest to understand the nature of dark matter and dark energy is a major focus of contemporary astrophysical and cosmological research. Various experiments, including those involving particle physics and astronomical observations, aim to detect or constrain the properties of dark matter. The nature of dark energy, however, remains one of the most profound mysteries in cosmology, with implications for the ultimate fate and structure of the universe.