Precision mass measurements of magnesium isotopes and implications for the validity of the isobaric mass multiplet equation

M. Brodeur, A. A. Kwiatkowski, O. M. Drozdowski, C. Andreoiu, D. Burdette, A. Chaudhuri, U. Chowdhury, A. T. Gallant, A. Grossheim, G. Gwinner, H. Heggen, J. D. Holt, R. Klawitter, J. Lassen, K. G. Leach, A. Lennarz, C. Nicoloff, S. Raeder, B. E. Schultz, S. R. Stroberg, A. Teigelhöfer, R. Thompson, M. Wieser, and J. Dilling
Phys. Rev. C 96, 034316 – Published 18 September 2017

Abstract

If the mass excess of neutron-deficient nuclei and their neutron-rich mirror partners are both known, it can be shown that deviations of the isobaric mass multiplet equation (IMME) in the form of a cubic term can be probed. Such a cubic term was probed by using the atomic mass of neutron-rich magnesium isotopes measured using the TITAN Penning trap and the recently measured proton-separation energies of Cl29 and Ar30. The atomic mass of Mg27 was found to be within 1.6σ of the value stated in the Atomic Mass Evaluation. The atomic masses of Mg28,29 were measured to be both within 1σ, while being 7 and 33 times more precise, respectively. Using the Mg29 mass excess and previous measurements of Cl29, we uncovered a cubic coefficient of d=28(7)keV, which is the largest known cubic coefficient of the IMME. This departure, however, could also be caused by experimental data with unknown systematic errors. Hence there is a need to confirm the mass excess of S28 and the one-neutron separation energy of Cl29, which have both come from a single measurement. Finally, our results were compared with ab initio calculations from the valence-space in-medium similarity renormalization group, resulting in a good agreement.

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  • Received 21 July 2017

DOI:https://doi.org/10.1103/PhysRevC.96.034316

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

M. Brodeur1,*, A. A. Kwiatkowski2,3, O. M. Drozdowski2,4, C. Andreoiu5, D. Burdette1, A. Chaudhuri2,†, U. Chowdhury2,6,7, A. T. Gallant2,8,9, A. Grossheim2, G. Gwinner7, H. Heggen2, J. D. Holt2, R. Klawitter2,10, J. Lassen2,7, K. G. Leach2,5,11, A. Lennarz2,12, C. Nicoloff1,13, S. Raeder2, B. E. Schultz2, S. R. Stroberg2, A. Teigelhöfer2,7, R. Thompson14, M. Wieser14, and J. Dilling2,8

  • 1Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
  • 2TRIUMF, Vancouver, British Columbia V6T 2A3, Canada
  • 3Department of Physics, Texas A&M University, College Station, Texas 77843, USA
  • 4Institute for Theoretical Physics, Universität Heidelberg, Philosophenweg 12, D-69120, Germany
  • 5Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
  • 6SNOLAB, Lively, Ontario P3Y 1N2, Canada
  • 7Department of Physics and Astronomy, University of Manitoba, Winnipeg, Manitoba R3T 2N2, Canada
  • 8Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
  • 9Physical and Life Science Directorate, Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 10Max-Planck-Institut für Kernphysik, D-69117 Heidelberg, Germany
  • 11Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA
  • 12Institut für Kernphysik, Westfälische Wilhelms-Universität, D-48149 Münster, Germany
  • 13Department of Physics, Wellesley College, Wellesley, Massachusetts 02481, USA
  • 14Department of Physics and Astronomy, University of Calgary, Alberta T2N 1N4, Canada

  • *mbrodeur@nd.edu
  • Present address: Canadian Nuclear Laboratories, Chalk River, Ontario K0J 1J0, Canada.

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Vol. 96, Iss. 3 — September 2017

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