Author:
Fiebiger Stefan,Baramsai Bayarbadrakh,Couture Aaron,Krtička Milan,Mosby Shea,O’Donnell John,Reifarth René,Rusev Gencho,Ullmann John,Weigand Mario,Wolf Clemens
Abstract
AbstractThe neutron capture cross section of $$^{83}$$
83
Kr has been measured via the time-of-flight technique between 25 meV and 500 keV. The experiment used the DANCE array at the Los Alamos National Laboratory. Maxwellian Averaged Cross Sections have been derived for a range of stellar temperatures and are found to be in good agreement with previous data. The impact of the new cross sections on stellar nucleosynthesis has been investigated.
Funder
FP7 Ideas: European Research Council
Grantová Agentura Ceské Republiky
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics