Abstract
The masses of very neutron-deficient nuclides close to the astrophysical - and -process paths have been determined with the Penning trap facilities JYFLTRAP at JYFL/Jyväskylä and SHIPTRAP at GSI/Darmstadt. Isotopes from yttrium () to palladium () have been produced in heavy-ion fusion-evaporation reactions. In total, 21 nuclides were studied, and almost half of the mass values were experimentally determined for the first time: , , , and . For the , () high-spin state, a first direct mass determination was performed. Relative mass uncertainties of typically were obtained. The impact of the new mass values has been studied in -process nucleosynthesis calculations. The resulting reaction flow and the final abundances are compared with those obtained with the data of the Atomic Mass Evaluation 2003.
5 More- Received 15 August 2008
DOI:https://doi.org/10.1103/PhysRevC.78.054310
©2008 American Physical Society