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Explore the theoretical foundations of core-collapse supernova explosions in this 47-minute conference talk delivered by Adam Burrows from Princeton University at the Kavli Institute for Theoretical Physics. Delve into the complex physics governing how massive stars end their lives through catastrophic core collapse, examining the mechanisms that drive these spectacular stellar explosions. Learn about the theoretical models that explain the transition from stellar core collapse to supernova explosion, including the role of neutrinos, shock waves, and nuclear physics in determining explosion outcomes. Understand how these theoretical frameworks connect to observational evidence from gravitational wave detections, stellar surveys, and transient observations that are revealing new insights into the stellar mass black hole population. Gain insights into the computational challenges and recent advances in supernova theory that help explain the diverse outcomes of massive star death, from successful explosions to black hole formation.
