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Collaborating directly with the experimental team, we integrate astrophysics, particle physics, and string theory with observational data to explore gravity and the formation and development of our cosmos. In cosmology and astrophysics, Einstein's General Theory of Relativity (GR) serves as the cornerstone for diverse phenomena, ranging from universe modeling to black hole collisions. Our team leads in applying numerical GR to analyze gravitational wave patterns from merging black holes and neutron stars, spacetime characteristics near the big bang, and aspects of string theory. Three decades ago, our group initiated research on large-scale cosmic structures, and we remain at the forefront of developing theories about their origins. Key components of this research involve the experimental team's measurements of the 2.725 K cosmic microwave background, extensive galaxy observations, and data from the Sloan Digital Sky Survey, operated by the adjacent Department of Astrophysical Sciences.