830 citations · 1.1k across the 19 of their papers we have counts for
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Cross section measurements of -induced reactions on Mo and Sn for -process studies
W. Rapp, I. Dillmann, F. Käppeler +5
The Mo()Ru, Mo()Ru, and Sn()Te cross sections were measured at the upper end of the -process Gamow window between 8.2…
New Stellar Cross Sections and The "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars"
I. Dillmann, R. Plag, C. Domingo-Pardo +4
Since April 2005 a regularly updated stellar neutron cross section compilation is available online at http://nuclear-astrophysics.fzk.de/kadonis. This online-database is called the…
First measurements of the total and partial stellar cross section to the -process branching-point Se
I. Dillmann, M. Heil, F. Käppeler +7
Although Se represents an important branching in the weak s process, the stellar neutron capture cross sections to this isotope have not yet been measured experimentally. In…
-Process simulations with a modified reaction library
I. Dillmann, T. Rauscher, M. Heil +3
We have performed -process simulations with the most recent stellar cross sections from the "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" project (versi…
(n,) Cross Sections of Light p Nuclei -- Towards an Updated Database for the p Process
I. Dillmann, M. Heil, F. Käppeler +3
The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small amount of stable isotopes on the proton-rich side cannot be made by neutron capt…
KADoNiS- The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars
I. Dillmann, M. Heil, F. Käppeler +3
The "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" (KADoNiS) project is an online database for experimental cross sections relevant to the s process and p process.…
Experimental (n,) cross sections of the p-process nuclei Se and Sr
I. Dillmann, M. Heil, F. Käppeler +2
The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small amount of stable isotopes on the proton-rich side cannot be made by neutron capt…