Proton-rich nucleosynthesis and nuclear physics
Rauscher, T. and Froehlich, C.
(2012)
Proton-rich nucleosynthesis and nuclear physics.
In: International Symposium on Origin of Matter and Evolutions of Galaxies (OMEG), 2011-11-14 - 2011-11-17.
Although the detailed conditions for explosive nucleosynthesis are derived from astrophysical modeling, nuclear physics determines fundamental patterns in abundance yields, not only for equilibrium processes. Focussing on the nu p- and the gamma-process, general nucleosynthesis features within the range of astrophysical models, but (mostly) independent of details in the modelling, are presented. Remaining uncertainties due to uncertain Q-values and reaction rates are discussed.
Item Type | Conference or Workshop Item (Other) |
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Keywords | nu-wind, core-collapse supernovae, supernovae, nu p-process, gamma-process, nucleosynthesis, reaction-rates, p-process |
Date Deposited | 15 May 2025 16:32 |
Last Modified | 10 Jul 2025 23:30 |
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picture_as_pdf - 1304.0929v1.pdf
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