Explodability criteria for the neutrino-driven supernova mechanism
Massive stars undergoing iron core-collapse at the end of their evolution terminate their lives either as successful or failed supernovae (SNe). The physics of core-collapse supernovae (CCSNe) is complex and understanding it requires computationally expensive simulations. Therefore, using these simu...
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| Main Authors: | , , , , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
August 2025
|
| In: |
Astronomy and astrophysics
Year: 2025, Volume: 700, Pages: 1-27 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/202554931 |
| Online Access: | Verlag, kostenfrei, Volltext: https://doi.org/10.1051/0004-6361/202554931 Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2025/08/aa54931-25/aa54931-25.html |
| Author Notes: | K. Maltsev, F.R.N. Schneider, I. Mandel, B. Müller, A. Heger, F.K. Röpke, and E. Laplace |
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Explodability criteria for the neutrino-driven supernova mechanism
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