Explodability criteria for the neutrino-driven supernova mechanism
Massive stars undergoing iron core collapse at the end of their evolution terminate their lives either in successful or failed supernovae (SNe). The physics of core collapse supernovae (CCSNe) is complex, and their understanding requires computationally expensive simulations. The sampling of large,...
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| Main Authors: | , , , , , , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
31 Mar 2025
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| In: |
Arxiv
Year: 2025, Pages: 1-25 |
| DOI: | 10.48550/arXiv.2503.23856 |
| Online Access: | Verlag, kostenfrei, Volltext: https://doi.org/10.48550/arXiv.2503.23856 Verlag, kostenfrei, Volltext: http://arxiv.org/abs/2503.23856 |
| Author Notes: | K. Maltsev, F.R.N. Schneider, I. Mandel, B. Müller, A. Heger, F.K. Röpke, E. Laplace |
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