@inproceedings{397cf6951b304fd5bb50bf6768274618,
title = "Reaction Rate Uncertainties and the nu p-Process",
abstract = "Current hydrodynamical simulations of core collapse supernovae find proton-rich early ejecta. At the same time, the models fail to eject neutron-rich matter, thus leaving the origin of the main r-process elements unsolved. However, the proton-rich neutrino-driven winds from supernovae have been identified as a possible production site for light n-capture elements beyond iron ( such as Ge, Sr, Y, Zr) through the nu p-process. The detailed nucleosynthesis patterns of the nu p-process depend on the hydrodynamic conditions and the nuclear reaction rates of key reactions. We investigate the impact of reaction rate uncertainties on the nu p-process nucleosynthesis.",
keywords = "nu-wind, core-collapse supernovae, nu p-process, nucleosynthesis, NUCLEI, MASS, TABLES",
author = "C. Froehlich and T. Rauscher",
year = "2012",
doi = "10.1063/1.4763400",
language = "English",
isbn = "978-0-7354-1096-1",
series = "AIP Conf Procs",
publisher = "American Institute of Physics (AIP)",
pages = "232--239",
editor = "S. Kubono",
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",
}