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Neutron activations for lower s-process temperatures.
- Source :
- EPJ Web of Conferences; 3/22/2023, Vol. 279, p1-4, 4p
- Publication Year :
- 2023
-
Abstract
- The slow neutron capture process produces heavy elements in different stellar sites at different temperatures. Neutron capture cross sections for stellar temperatures between k<subscript>B</subscript>T = 5 keV and k<subscript>B</subscript>T = 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 k<subscript>B</subscript>T = 25 keV. We developed a new method to measure neutron capture cross sections at k<subscript>B</subscript>T = 6 keV. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 21016275
- Volume :
- 279
- Database :
- Complementary Index
- Journal :
- EPJ Web of Conferences
- Publication Type :
- Conference
- Accession number :
- 162589917
- Full Text :
- https://doi.org/10.1051/epjconf/202327906011