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Explore the revolutionary discoveries in stellar mass black hole populations through this 42-minute conference talk examining how gravitational wave detections, Gaia observations, microlensing surveys, and time domain studies are unveiling previously unknown black hole populations. Learn about dormant black holes in detached binary systems, isolated black holes detected through microlensing, and transient events marking black hole formation or stellar interactions that complement traditional X-ray and radio survey discoveries. Examine the complete lifecycle of stellar black holes from their massive star progenitors through core collapse and associated transients to their afterlives as dormant or accreting objects and potential gravitational wave merger sources. Discover how these new observational capabilities are compelling researchers to reassess theoretical understanding of black hole evolution and develop new strategies for answering fundamental questions about stellar black hole populations across different redshifts and metallicity environments.
