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Neutron-induced cross sections

From raw data to astrophysical rates

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Abstract.

Neutron capture cross sections are one of the most important nuclear inputs to models of stellar nucleosynthesis of the elements heavier than iron. The activation technique and the time-of-flight method are mostly used to determine the required data experimentally. Recent developments of experimental techniques allow for new experiments on radioactive isotopes. Monte Carlo based analysis methods give new insights into the systematic uncertainties of previous measurements. We present an overview over the state-of-the-art experimental techniques, a detailed new evaluation of the 197Au(n,\(\gamma\)) cross section in the keV-regime and the corresponding re-evaluation of 63 more isotopes, which have been measured in the past relative to the gold cross section.

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Authors and Affiliations

  1. Goethe University Frankfurt am Main, Frankfurt, Germany

    René Reifarth, Philipp Erbacher, Stefan Fiebiger, Kathrin Göbel, Tanja Heftrich, Nadine Klapper, Deniz Kurtulgil, Christoph Langer, Benedikt Thomas & Mario Weigand

  2. GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany

    Michael Heil

  3. Karlsruhe Institute of Technology, Karlsruhe, Germany

    Franz Käppeler

  4. School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK

    Claudia Lederer-Woods

  5. ENEA, Bologna, Italy

    Alberto Mengoni

  6. INFN, Sezione di Bologna, Bologna, Italy

    Alberto Mengoni

  7. Frankfurt Institute for Advanced Studies, Frankfurt, Germany

    Stefan Schmidt

  8. University of Notre Dame, Notre Dame, IN, USA

    Michael Wiescher

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  1. René Reifarth
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  16. Michael Wiescher
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Correspondence to René Reifarth.

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Reifarth, R., Erbacher, P., Fiebiger, S. et al. Neutron-induced cross sections. Eur. Phys. J. Plus 133, 424 (2018). https://doi.org/10.1140/epjp/i2018-12295-3

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