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Explore the dynamical formation mechanisms of black hole binary systems in this 45-minute conference talk from the Kavli Institute for Theoretical Physics. Delve into how gravitational wave detections are transforming our understanding of stellar mass black hole populations, while examining new discoveries from Gaia observations of dormant black holes in detached binaries and microlensing studies of isolated black holes. Learn about the complex lifecycle of stellar black holes, from their massive star progenitors through core collapse and associated transients, to their evolution as dormant or accreting systems that may eventually merge as gravitational wave sources. Discover how time domain surveys are identifying transients that mark black hole formation and stellar companion interactions, revealing populations that complement traditional X-ray and radio survey findings. Gain insights into current observational and theoretical strategies being developed to address fundamental questions about stellar black hole evolution and the processes that lead to binary formation through dynamical assembly mechanisms.
