The Core Collapse Supernova Mechanism: Current Models, Gaps, and the Road Ahead
Anthony Mezzacappa

TL;DR
This paper reviews the progress and current challenges in modeling the core collapse supernova explosion mechanism, emphasizing recent advances in multidimensional simulations and the need for comprehensive inclusion of key physical components.
Contribution
It highlights the development of multidimensional supernova models and identifies the essential components required for realistic 3D simulations.
Findings
Recent models incorporate multidimensional effects and improved neutrino transport.
Key components for realistic models have been identified.
Including all critical components remains a significant challenge.
Abstract
The pursuit of the core collapse supernova explosion mechanism continues. While such efforts have been undertaken over the last four decades, it is only in the last decade that multidimensional models have been developed, and only in the last few years that significant components of supernova models, such as the neutrino transport, have been modeled with sufficient realism. We can now identify what are arguably the important components that must be included in any realistic three-dimensional supernova model. The challenge we now face is to include all of these in the models.
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae
