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The fields of Astrophysics and Cosmology explore the physical principles behind celestial phenomena and investigate the Universe's beginnings, development, makeup, and ultimate destiny. Our research team addresses some of physics' most challenging and profound unanswered questions. Most of the Universe's matter consists not of familiar standard model particles but of an enigmatic substance called dark matter. While we've observed dark matter's gravitational influence, understanding its true nature demands detecting how it interacts with ordinary matter. Just 15 years ago, scientists didn't recognize the primary component of the Universe's energy density. This mysterious dark energy manifests through the Universe's accelerating expansion and altered growth of mass disturbances. Unraveling dark energy's secrets will necessitate experiments capable of measuring its redshift-dependent effects with extraordinary accuracy. Contemporary cosmological theories depend on an early inflationary period to explain the horizon problem and initiate structure formation. Confirming cosmology's standard model requires detecting gravitational waves produced during this inflationary epoch.