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Explore the complex dynamics of star-black hole interactions within young stellar clusters through this 44-minute conference talk. Examine how gravitational wave detections are transforming our understanding of stellar mass black hole populations, while Gaia observations reveal dormant black holes in detached binary systems with stellar companions. Investigate how microlensing techniques probe otherwise unobservable isolated black holes, and discover how time domain surveys search for transients that mark black hole formation or stellar companion interactions. Learn about the emerging black hole population that complements the accreting black holes traditionally studied through X-ray and radio surveys. Delve into the complete lifecycle of stellar black holes, from the complicated evolution of their massive star progenitors through core collapse and associated transients, to their afterlives as dormant or accreting objects, and their potential finale as gravitational wave sources during mergers. Gain insights into the latest observational findings and theoretical strategies being developed to address fundamental questions about stellar black hole evolution within the context of young star cluster environments.
