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.

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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)
Identification Number	10.1063/1.4763376
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	22 Oct 2025 20:00