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Explore the latest discoveries in merging compact binary populations through this 44-minute conference talk that examines how gravitational wave detections are transforming our understanding of stellar mass black holes. Learn about the revolutionary insights from multiple detection methods including Gaia's observations of dormant black holes in detached binaries, microlensing studies of isolated black holes, and time domain surveys tracking transients that mark black hole formation and stellar interactions. Discover how these complementary detection techniques are revealing new populations that extend beyond the traditionally known accreting black holes from X-ray and radio surveys. Examine the complete lifecycle of stellar black holes, from their massive star progenitors through core collapse and associated transients, to their existence as dormant or accreting objects, and their potential fate as gravitational wave sources during merger events. Gain insights into current observational findings and emerging theoretical strategies being developed to address fundamental questions about stellar black hole evolution and population characteristics.
