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Mass measurements and evaluation around A = 22
Authors:M Mukherjee  D Beck  K Blaum  G Bollen  P Delahaye  J Dilling  S George  C Guénaut  F Herfurth  A Herlert  A Kellerbauer  H -J Kluge  U Köster  D Lunney  S Schwarz  L Schweikhard  C Yazidjian
Institution:1. GSI, Planckstra?e 1, 64291, Darmstadt, Germany
2. Insitute of Physics, Johannes Gutenberg-University, 55099, Mainz, Germany
3. NSCL, Michigan State University, East Lansing, 48824-1321, MI, USA
4. Physics Department, CERN, 1211, Genève, Switzerland
5. TRIUMF, V6T 2A3, British Columbia, Canada
6. CSNSM-IN2P3-CNRS, 91405, Orsay-Campus, France
7. Institute of Physics, Ernst-Moritz-Arndt-University, 17487, Greifswald, Germany
8. Institute of Physics, Ruprecht-Karls-University, 69120, Heidelberg, Germany
Abstract:Frequency ratio measurements with different combinations of the singly charged ions from 21, 22, 23Na , 22, 24Mg , and 37, 39K were performed at the on-line Penning trap mass spectrometer ISOLTRAP, CERN, Geneva. The masses and mass differences were deduced with a relative uncertainty of about or even below one part in 108 for the ions of interest using a least-squares analysis of all measured relations. The results have direct consequences for weak-interaction study as they give additional input to the test of CVC, and for nuclear astrophysics, because they help to establish the minimum observable signal for a NeNa cycle in a nova burst. We report here about the measurements and the detailed evaluation.
Keywords:21  10  Dr Binding energies and masses  26  30  -k Nucleosynthesis in novae  supernovae and other explosive environments  27  30  +t 20≤  A  38  32  10  Bi Atomic masses  mass spectra  abundances  and isotopes
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