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Mass measurements in the vicinity of the rp-process and the nu p-process paths with JYFLTRAP and SHIPTRAP

Authors :
Weber, C.
Elomaa, V. -V.
Ferrer, R.
Fröhlich, C.
Ackermann, D.
Äystö, J.
Audi, G.
Batist, L.
Blaum, K.
Block, M.
Chaudhuri, A.
Dworschak, M.
Eliseev, S.
Eronen, T.
Hager, U.
Hakala, J.
Herfurth, F.
Heßberger, F. P.
Hofmann, S.
Jokinen, A.
Kankainen, A.
Kluge, H. -J.
Langanke, K.
Martín, A.
Martínez-Pinedo, G.
Mazzocco, M.
Moore, I. D.
Neumayr, J. B.
Novikov, Yu. N.
Penttilä, H.
Plaß, W. R.
Popov, A. V.
Rahaman, S.
Rauscher, T.
Rauth, C.
Rissanen, J.
Rodríguez, D.
Saastamoinen, A.
Scheidenberger, C.
Schweikhard, L.
Seliverstov, D. M.
Sonoda, T.
Thielemann, F. -K.
Thirolf, P. G.
Vorobjev, G. K.
Publication Year :
2008
Publisher :
arXiv, 2008.

Abstract

The masses of very neutron-deficient nuclides close to the astrophysical rp- and nu p-process paths have been determined with the Penning trap facilities JYFLTRAP at JYFL/Jyv\"askyl\"a and SHIPTRAP at GSI/Darmstadt. Isotopes from yttrium (Z = 39) to palladium (Z = 46) 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: 88Tc, 90-92Ru, 92-94Rh, and 94,95Pd. For the 95Pdm, (21/2^+) high-spin state, a first direct mass determination was performed. Relative mass uncertainties of typically $\delta m / m = 5 \times 10^{-8}$ were obtained. The impact of the new mass values has been studied in nu p-process nucleosynthesis calculations. The resulting reaction flow and the final abundances are compared to those obtained with the data of the Atomic Mass Evaluation 2003.<br />Comment: 21 pages, 12 figures, 2 tables, submitted to Phys. Rev. C

Details

Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....f19fabb5506bd90fb6919e534f0fe094
Full Text :
https://doi.org/10.48550/arxiv.0808.4065