Testing refined shell-model interactions in the sd shell: Coulomb excitation of 26Na
Siebeck, B., Seidlitz, M., Blazhev, A., Reiter, P., Altenkirch, R., Bauer, C., Butler, P. A., De Witte, H., Elseviers, J., Gaffney, L. P., Hess, H., Huyse, M., Kröll, T., Lutter, R., Pakarinen, J., Pietralla, N., Radeck, F., Scheck, M., Schneiders, D., . . . Wenander, F. (2015). Testing refined shell-model interactions in the sd shell: Coulomb excitation of 26Na. Physical Review C, 91(1), Article 014311. https://doi.org/10.1103/PhysRevC.91.014311
Published inPhysical Review C
Hess, H. |
Warr, N. |
© Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License.
Background: Shell-model calculations crucially depend on the residual interaction used to approximate the nucleon-nucleon interaction. Recent improvements to the empirical universal sd interaction (USD) describing nuclei within the sd shell yielded two new interactions—USDA and USDB—causing changes in the theoretical description of these nuclei. Purpose: Transition matrix elements between excited states provide an excellent probe to examine the underlying shell structure. These observables provide a stringent test for the newly derived interactions. The nucleus 26Na with 7 valence neutrons and 3 valence protons outside the doubly-magic 16O core is used as a test case. Method: A radioactive beam experiment with 26Na (T1/2 = 1,07s) was performed at the REX-ISOLDE facility (CERN) using Coulomb excitation at safe energies below the Coulomb barrier. Scattered particles were detected with an annular Si detector in coincidence with γ rays observed by the segmented MINIBALL array. Coulomb excitation cross sections of the beam have been obtained by normalization to the well known Coulomb excitation cross sections of the 104Pd target. Results: The observation of three γ -ray transitions in 26Na together with available spectroscopic data allows us to determine E2- and M1-transitional matrix elements. Results are compared to theoretical predictions. Conclusion: The improved theoretical description of 26Na could be validated. Remaining discrepancies between experimental data and theoretical predictions indicate the need for future experiments and possibly further theoretical improvements. ...
PublisherAmerican Physical Society
ISSN Search the Publication Forum0556-2813
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Except where otherwise noted, this item's license is described as © Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License.
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