Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data.

@article{Rauscher2013ConstrainingTA,
  title={Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data.},
  author={Thomas Rauscher and Nicolas Dauphas and Iris Dillmann and Carla Fr{\"o}hlich and Zs. F{\"u}l{\"o}p and Gy. Gy{\"u}rky},
  journal={Reports on progress in physics. Physical Society},
  year={2013},
  volume={76 6},
  pages={
          066201
        }
}
A small number of naturally occurring, proton-rich nuclides (the p-nuclei) cannot be made in the s- and r-processes. Their origin is not well understood. Massive stars can produce p-nuclei through photodisintegration of pre-existing intermediate and heavy nuclei. This so-called γ-process requires high stellar plasma temperatures and occurs mainly in explosive O/Ne burning during a core-collapse supernova. Although the γ-process in massive stars has been successful in producing a large range of… 
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A number of naturally occurring, proton-rich nuclides (the p-nuclei) cannot be made in the s- and r-process. It has been found that massive stars can produce p-nuclei through photodisintegration of
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