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Explore how black hole spins serve as diagnostic tools for understanding black hole formation and evolution within young massive stellar clusters in this 17-minute conference talk. Examine the relationship between spin measurements and the growth mechanisms of black holes in dense stellar environments, where dynamical interactions and stellar evolution processes create unique conditions for black hole development. Learn about the theoretical frameworks connecting spin properties to formation channels, including primordial black hole formation, stellar collapse scenarios, and accretion-driven growth in cluster environments. Discover how observational data from gravitational wave detections, particularly those revealing spin-orbit misalignments and spin magnitudes, provide insights into the evolutionary pathways of black holes in these extreme stellar nurseries. Understand the implications of spin measurements for distinguishing between different formation mechanisms and constraining models of black hole population synthesis in young massive clusters, where high stellar densities and frequent interactions shape the black hole demographic.
