Mass measurements of neutron-deficient nuclei and their implications for astrophysics |
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Authors: | A Kankainen Yu N Novikov H Schatz C Weber |
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Institution: | 1.Department of Physics,University of Jyv?skyl?,Jyv?skyl?,Finland;2.Petersburg Nuclear Physics Institute,Gatchina,Russia;3.GSI Helmholtzzentrum für Schwerionenforschung GmbH,Darmstadt,Germany;4.Department of Physics and Astronomy, National Superconducting Cyclotron Laboratory, and Joint Institute for Nuclear Astrophysics,Michigan State University,Michigan,USA;5.Faculty of Physics,Ludwig-Maximilians-Universit?t München,Garching,Germany |
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Abstract: | During the years 2005-2010 the double-Penning-trap mass spectrometer JYFLTRAP has been used to measure the masses of 90 ground
and 8 isomeric states of neutron-deficient nuclides with a typical precision of better than 10keV. The masses of 14 nuclides
-- 84Zr , 88, 89Tc , 90-92Ru , 92-94Rh , 94, 95Pd , 106, 108, 110Sb -- have been experimentally determined for the first time. This article gives an overview on these measurements and their
impact on the modeling of the astrophysical rp -process. |
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