Symplectic no-core shell-model approach to intermediate-mass nuclei

G. K. Tobin, M. C. Ferriss, K. D. Launey, T. Dytrych, J. P. Draayer, A. C. Dreyfuss, and C. Bahri
Phys. Rev. C 89, 034312 – Published 19 March 2014

Abstract

We present a microscopic description of nuclei in the intermediate-mass region, including the proximity to the proton drip line, based on a no-core shell model with a schematic many-nucleon long-range interaction with no parameter adjustments. The outcome confirms the essential role played by the symplectic symmetry to inform the interaction and the winnowing of shell-model spaces. We show that it is imperative that model spaces be expanded well beyond the current limits up through 15 major shells to accommodate particle excitations, which appear critical to highly deformed spatial structures and the convergence of associated observables.

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  • Received 10 November 2013
  • Revised 13 February 2014

DOI:https://doi.org/10.1103/PhysRevC.89.034312

©2014 American Physical Society

Authors & Affiliations

G. K. Tobin, M. C. Ferriss, K. D. Launey*, T. Dytrych, J. P. Draayer, and A. C. Dreyfuss

  • Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA

C. Bahri

  • Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556-5670, USA

  • *kristina@baton.phys.lsu.edu

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Vol. 89, Iss. 3 — March 2014

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