Shell-model Monte Carlo studies of neutron-rich nuclei in the 1s0d1p0f shells

D. J. Dean, M. T. Ressell, M. Hjorth-Jensen, S. E. Koonin, K. Langanke, and A. P. Zuker
Phys. Rev. C 59, 2474 – Published 1 May 1999
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Abstract

We demonstrate the feasibility of realistic shell-model Monte Carlo (SMMC) calculations spanning multiple major shells, using a realistic interaction whose bad saturation and shell properties have been corrected by a newly developed general prescription. Particular attention is paid to the approximate restoration of translational invariance. The model space consists of the full sdpf shells. We include in the study some well-known T=0 nuclei and several unstable neutron-rich ones around N=20,28. The results indicate that SMMC calculations can reproduce binding energies, B(E2) transitions, and other observables with an interaction that is practically parameter free. Some interesting insight is gained into the nature of deep correlations. The validity of previous studies is confirmed.

  • Received 16 November 1998

DOI:https://doi.org/10.1103/PhysRevC.59.2474

©1999 American Physical Society

Authors & Affiliations

D. J. Dean1, M. T. Ressell2,4, M. Hjorth-Jensen3, S. E. Koonin2, K. Langanke5, and A. P. Zuker6

  • 1Physics Division, Oak Ridge National Laboratory, P.O. Box 2008, Oak Ridge, Tennessee 37831Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennesseek 37996
  • 2W.K. Kellogg Radiation Laboratory, 106-38, California Institute of Technology, Pasadena, California 91125
  • 3Nordita, Blegdamsvej 17, DK-2100 Copenhagen Ø, DenmarkDepartment of Physics, University of Oslo, Norway
  • 4Astronomy and Astrophysics Center, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637
  • 5Institute for Physics and Astronomy, Aarhus University, Denmark
  • 6Institut de Recherches Subatomiques, Bâtiment 27, IN2P3-CNRS/Université Louis Pasteur Boîte Postal 28, F-67037 Strasbourg Cedex 2, France

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Vol. 59, Iss. 5 — May 1999

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