@inproceedings{dcce7cba8cc24233a1ae828a0696cfd1,
title = "Proton-rich nucleosynthesis and nuclear physics",
abstract = "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.",
keywords = "nu-wind, core-collapse supernovae, SUPERNOVAE, nu p-process, gamma-process, nucleosynthesis, REACTION-RATES, P-PROCESS",
author = "T. Rauscher and C. Froehlich",
year = "2012",
doi = "10.1063/1.4763376",
language = "English",
isbn = "978-0-7354-1096-1",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics (AIP)",
pages = "73--78",
editor = "S. Kubono and T. Hayakawa and T. Kajino and H. Miyatake and T. Motobayashi and K. Nomoto",
booktitle = "Origin of Matter and Evolution of Galaxies 2011",
address = "United States",
note = "International Symposium on Origin of Matter and Evolutions of Galaxies (OMEG) ; Conference date: 14-11-2011 Through 17-11-2011",
}