Physical Conditions for Synthesis of Sc, Ti, and V in Neutrino-driven Supernovae
We present the results of simulations of nucleosynthesis in a core-collapse supernova including the neutrino process. Using the Si layer of a 13 M _⊙ zero-metal progenitor as the initial composition, we calculate the nucleosynthesis by adopting the temperature, density, neutrino flux, and duration o...
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| Huvudupphov: | , , , , |
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| Materialtyp: | Artigo |
| Språk: | Inglês |
| Utgiven: |
IOP Publishing
2026-01-01
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| Serie: | The Astrophysical Journal |
| Ämnen: | |
| Länkar: | https://doi.org/10.3847/1538-4357/ae2fbc |
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