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NSR database version of May 3, 2024.

Search: Author = G.Merz

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2020SU17      Astrophys.J. 898, 5 (2020)

S.K.Subedi, Z.Meisel, G.Merz

Sensitivity of ⁴⁴Ti and ⁵⁶Ni Production in Core-collapse Supernova Shock-driven Nucleosynthesis to Nuclear Reaction Rate Variations

NUCLEAR REACTIONS ¹³N, ¹⁷F, ⁵²Fe, ⁵⁶Ni(α, p), ⁵⁷Ni(n, p), ⁵⁶Co(p, n), ³⁹K, ⁴⁷V, ⁵²Mn, ⁵⁷Co(p, γ), ³⁹K(p, α), E not given; calculated reaction rates.

doi: 10.3847/1538-4357/ab9745
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