Phys. Rev. Lett.
106,
122501
(2011)
[5 pages]
Mass Measurements of Very Neutron-Deficient Mo and Tc Isotopes and Their Impact on rp Process Nucleosynthesis
E. Haettner et al.
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E. Haettner1,2,*, D. Ackermann2, G. Audi3, K. Blaum4, M. Block2, S. Eliseev2,†, T. Fleckenstein1, F. Herfurth2, F. P. Heßberger2, S. Hofmann2, J. Ketelaer5,†, J. Ketter4, H.-J. Kluge2, G. Marx6, M. Mazzocco7, Yu. N. Novikov2,8, W. R. Plaß1,2, S. Rahaman9,‡, T. Rauscher10, D. Rodríguez11, H. Schatz12, C. Scheidenberger1,2, L. Schweikhard6, B. Sun1,13, P. G. Thirolf14, G. Vorobjev2,8, M. Wang15, and C. Weber9,§
1II. Physikalisches Institut, Justus-Liebig-Universität, 35392 Gießen, Germany 2GSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, Germany 3CSNSM-IN2P3-CNRS, 91405 Orsay-Campus, France 4Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany 5Institut für Physik, Johannes Gutenberg-Universität, 55128 Mainz, Germany 6Institut für Physik, Ernst-Moritz-Arndt-Universität, 17487 Greifswald, Germany 7Dipartimento di Fisica and INFN Sezione di Padova, 35131 Padova, Italy 8Petersburg Nuclear Physics Institute, 188300 Gatchina, St. Petersburg, Russia 9Department of Physics, University of Jyväskylä, 40014 Jyväskylä, Finland 10Department of Physics, University of Basel, 4056 Basel, Switzerland 11Universidad de Granada, 18071 Granada, Spain 12Department of Physics and Astronomy, NSCL, and JINA, Michigan State University, East Lansing, Michigan 48824-1321, USA 13School of Physics and Nuclear Energy Engineering, Beihang University, 100191 Beijing, People’s Republic of China 14Fakultät für Physik, Ludwig-Maximilians-Universität, 85748 Garching, Germany 15Institute of Modern Physics, Lanzhou, People’s Republic of China
Received 26 August 2010; published 21 March 2011
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The masses of ten proton-rich nuclides, including the N=Z+1 nuclides 85Mo and 87Tc, were measured with the Penning trap mass spectrometer SHIPTRAP. Compared to the Atomic Mass Evaluation 2003 a systematic shift of the mass surface by up to 1.6 MeV is observed causing significant abundance changes of the ashes of astrophysical x-ray bursts. Surprisingly low α separation energies for neutron-deficient Mo and Tc are found, making the formation of a ZrNb cycle in the rp process possible. Such a cycle would impose an upper temperature limit for the synthesis of elements beyond Nb in the rp process.
© 2011 American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.106.122501
DOI:
10.1103/PhysRevLett.106.122501
PACS:
21.10.Dr, 07.75.+h, 26.30.Ca, 27.50.+e
*emma.k.haettner@physik.uni-giessen.de †Present address: Max-Planck-Institut für Kernphysik, 69117 Heidelberg, Germany ‡Present address: LANL, Physics Division, P-23, MS-H803, Los Alamos 87545, USA §Present address: Fakultät für Physik, Ludwig-Maximilians-Universität, 85748 Garching, Germany
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