empirical estimation of astrophysical photodisintegration rates of 106cd

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ID: 237778
2017
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Abstract
It has been noted in previous experiments that the ratio between the photoneutron and photoproton disintegration channels of 106Cd might be considerably different from predictions of statistical models. The thresholds of these reactions differ by several MeV and the total astrophysical rate of photodisintegration of 106Cd, which is mostly produced in photonuclear reactions during the p-process nucleosynthesis, might be noticeably different from the calculated value. In this work the bremsstrahlung beam of a 55.6 MeV microtron and the photon activation technique is used to measure yields of photonuclear reaction products on isotopically-enriched cadmium targets. The obtained results are compared with predictions of statistical models. The experimental yields are used to estimate photodisintegration reaction rates on 106Cd, which are then used in nuclear network calculations to examine the effects of uncertainties on the produced abundences of p-nuclei.
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s.s.2017epjempirical Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Belyshev S.S.;Kuznetsov A.A.;Stopani K.A.
Journal utilitas mathematica
Year 2017
DOI
10.1051/epjconf/201714601011
URL
https://doi.org/10.1051/epjconf/201714601011
Keywords
physics

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