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Explore the revolutionary discoveries in stellar mass black hole populations through this 43-minute conference talk examining the triple connection between black hole mergers, electromagnetic counterparts, and galactic black holes. Learn how gravitational wave detections are transforming our understanding of black hole populations, while Gaia observations reveal new dormant black holes in detached binary systems with stellar companions. Discover how microlensing techniques probe isolated black holes that would otherwise remain unobservable, and understand how time domain surveys search for transients that mark either the birth of black holes or their interactions with stellar companions. Examine how these complementary detection methods are unveiling a new population of black holes that extends beyond the accreting black holes traditionally identified through X-ray and radio surveys. Assess current understanding of the complete lifecycle of stellar black holes, from the complex evolution of their massive star progenitors through core collapse and associated transients, to their afterlives as either dormant or accreting systems, and their potential finale as gravitational wave sources during merger events. Gain insights into the latest observational findings and theoretical strategies being developed to address fundamental questions about stellar black hole evolution and behavior.
