Investigation of -induced reactions on 127 I for the astrophysical process

@inproceedings{Kiss2012InvestigationO,
  title={Investigation of -induced reactions on 127 I for the astrophysical process},
  author={G{\'a}bor Gyula Kiss and Tam'as Szucs and Zs. Torok and Zeren Korkulu and Gy. Gyurky and Z. Hal'asz and Zs. Fulop and E. Somorjai and Thomas Rauscher},
  year={2012}
}
BACKGROUND: The γ process in core-collapse supernova explosions is thought to explain the origin of proton-rich isotopes between Se and Hg, the so-called p nuclei. The majority of the reaction rates for γ-process reaction network studies has to be predicted in Hauser-Feshbach statistical model calculations. Recent investigations showed problems in the prediction of α widths at astrophysical energies. This impacts the reliability of abundance predictions in the upper mass range of the p nuclei… 
The activation method for cross section measurements in nuclear astrophysics
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