Sensitivity study for s process nucleosynthesis in AGB stars
  In this paper we present a large-scale sensitivity study of reaction rates in the main component of the $s$ process. The aim of this study is to identify all rates, which have a global effect on the $s$ process abundance distribution and the three most important rates for the production of each isotope. We have performed a sensitivity study on the radiative $^{13}$C-pocket and on the convective thermal pulse, sites of the $s$ process in AGB stars. We identified 22 rates, which have the highest impact on the $s$-process abundances in AGB stars. 
A. Koloczek, B. Thomas, J. Glorius, R. Plag, M. Pignatari, R.   Reifarth, C. Ritter, S. Schmidt, K. Sonnabend
astro-ph.SR