Abstract
The explosion mechanism of core-collapse supernovae is a long-standing problem in stellar astrophysics. We briefly outline the main contenders for a solution and review recent efforts to model core-collapse supernova explosions by means of multi-dimensional simulations. Focusing on the neutrino-driven mechanism, we summarize currents efforts to predict supernova explosion and remnant properties.
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APA
Müller, B. (2016). The core-collapse supernova explosion mechanism. Proceedings of the International Astronomical Union, 12(S329), 17–24. https://doi.org/10.1017/s1743921317002575
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