Mass measurements and evaluation around A = 22 |
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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 |
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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
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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. |
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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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