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 10 keV. 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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Kankainen, A., Novikov, Y.N., Schatz, H., Weber, C. (2012). Mass measurements of neutron-deficient nuclei and their implications for astrophysics. In: Äystö, J., Eronen, T., Jokinen, A., Kankainen, A., Moore, I.D., Penttilä, H. (eds) Three decades of research using IGISOL technique at the University of Jyväskylä. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-5555-0_27
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