The Emerging Detailed Theory of Core-Collapse Supernova Explosions

Explore the latest advancements in core-collapse supernova theory through this comprehensive physics colloquium. Delve into the findings from over 20 state-of-the-art 3D simulations, revealing correlations between supernova observables and progenitor core structures. Discover the relationships between explosion energy, neutron star birth masses, chemical element yields, and pulsar kicks. Examine the connection between explosion energy and progenitor mantle binding energy, suggesting self-regulation in these cosmic events. Investigate the correlation between explosion energy and asymmetry measures, such as ejecta mass dipole. Gain insights into the current state of supernova theory, its qualitative solutions, and the challenges that remain in quantitatively explaining diverse supernova observations. Conclude by exploring potential paths forward in achieving a more robust understanding of these spectacular stellar explosions.