Determination of the Maxwellian averaged cross-section of the reaction 35Cl(n,γ)36Cl
Determination of the Maxwellian averaged cross-section of the reaction 35Cl(n,γ)36Cl
Pavetich, S.; Akhmadaliev, S.; Dillmann, I.; Halfon, S.; Heftrich, T.; Käppeler, F.; Lederer, C.; Martschini, M.; Merchel, S.; Paul, M.; Reifarth, R.; Rugel, G.; Steier, P.; Tessler, M.; Wallner, A.; Weigand, M.; Weissman, L.
Abstract
Routine measurements of 36Cl at the Dresden Accelerator Mass Spectrometry (DREAMS) facility have resulted in an astrophysical application: the determination of the Maxwellian averaged cross-section (MACS) of the reaction 35Cl(n,γ)36Cl. As 35Cl acts as a neutron poison in the nucleosynthesis processes during later burning phases of stars, the reaction is important for astrophysical calculations of elemental abundances. The neutron irradiations with a quasi Maxwell Boltzmann spectrum for the production of 36Cl were performed at the Karlsruhe Institute of Technology and the Soreq Applied Research Accelerator Facility. AMS measurements were performed at VERA and DREAMS and are planned at the Australian National University in 2015. Acknowledgement: Alberto Mengoni, CERN.
Keywords: Accelerator Mass Spectrometry; DREAMS; astrophysics; 36Cl
Beteiligte Forschungsanlagen
- Ionenstrahlzentrum DOI: 10.17815/jlsrf-3-159
Verknüpfte Publikationen
- DOI: 10.17815/jlsrf-3-159 is cited by this (Id 22923) publication
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Vortrag (Konferenzbeitrag)
DPG-Frühjahrstagung der Sektion AMOP (SAMOP), 23.-27.03.2015, Heidelberg, Deutschland
Permalink: https://www.hzdr.de/publications/Publ-22923