Author:
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
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 kBT = 6 keV.
Reference5 articles.
1. Neutron reactions in astrophysics
2. Neutron-induced cross sections
3. Quasistellar spectrum for neutron activation measurements atkT=5keV
4. PINO—a tool for simulating neutron spectra resulting from the 7Li(p,n) reaction
5. Dillmann I., Plag R., Käppeler F., Rauscher T., KADoNiS v0.3 The third update of the “Karlsruhe Astrophysical Database of Nucleosynthesis in Stars, in Proceeding of the workshop EFNUDAT Fast Neutrons scientific workshop on neutron measurements, theory & applications (2009), Geel, Belgium
Cited by
1 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献