The cosmic web is a large-scale structure that describes the distribution of matter in the universe. It is a fundamental concept in cosmology and provides a framework for understanding how galaxies and galaxy clusters are arranged in the cosmos. The formation and evolution of the cosmic web are driven by the gravitational interaction of dark matter, which makes up the majority of the universe’s matter content. The ordinary matter (baryonic matter), including galaxies and gas, is influenced by the gravitational pull of dark matter and tends to align along the filaments. Understanding the cosmic web is crucial for cosmologists as it provides insights into the large-scale structure of the universe, the distribution of matter, and the formation of galaxies and galaxy clusters.