2023
DOI: 10.1051/epjconf/202327906011
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Neutron activations for lower s-process temperatures

Abstract: The slow neutron capture process produces heavy elements in different stellar sites at different temperatures. Neutron capture cross sections for stellar temperatures between kBT = 5 keV and kBT = 100 keV are crucial for a quantitative understanding of the s-process abundance distribution. Over the last decade activation measurements were performed at the Goethe University Frankfurt to study cross sections at a temperature of kBT = 25 keV. We developed a new method to measure neutron capture cross sections at … Show more

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“…We are currently investigating the possibility to extend this methodology to lower energies between 5 keV and 25 keV. The first results of this innovative methodology are presented in the proceeding of Tanja Heftrich, included in this conference [2].…”
Section: Discussionmentioning
confidence: 99%
“…We are currently investigating the possibility to extend this methodology to lower energies between 5 keV and 25 keV. The first results of this innovative methodology are presented in the proceeding of Tanja Heftrich, included in this conference [2].…”
Section: Discussionmentioning
confidence: 99%