Issue |
EPJ Web Conf.
Volume 279, 2023
Nuclear Physics in Astrophysics – X (NPA-X 2022)
|
|
---|---|---|
Article Number | 06011 | |
Number of page(s) | 4 | |
Section | s process | |
DOI | https://doi.org/10.1051/epjconf/202327906011 | |
Published online | 22 March 2023 |
https://doi.org/10.1051/epjconf/202327906011
Neutron activations for lower s-process temperatures
1 Goethe University Frankfurt, Frankfurt, Germany
2 Jordan Atomic Energy Commission/Jordan Research and Training Reactor
3 Facility for Antiproton and Ion Research in Europe GmbH (FAIR GmbH), Darmstadt, Germany
* e-mail: heftrich@iap.uni-frankfurt.de
Published online: 22 March 2023
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 kBT = 6 keV.
© The Authors, published by EDP Sciences, 2023
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