Neutron activations for lower s-process temperatures
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...
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Bibliographic Details
Main Authors: |
Heftrich Tanja,
Al-Khasawleh Kafa,
Borzek Sandra,
Brückner Benjamin,
Dellmann Sophia Florence,
Dogan Ozan Can,
El Mard Asmaa,
Erbacher Philipp,
Gail Madeleine,
Göbel Kathrin,
Habermehl Fabian,
Heybeck Benedict,
Kisselbach Timo,
Kurtulgil Deniz,
Mourad Rim,
Reich Markus,
Reifarth René,
Sheriff Silas,
Staab Tom,
Volknandt Meiko,
Weigand Mario |
Format: | Article
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Language: | English |
Published: |
EDP Sciences
2023-01-01
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Series: | EPJ Web of Conferences
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Online Access: | https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_06011.pdf
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