Probing Configuration Mixing in Be12 with Gamow-Teller Transition Strengths

R. Meharchand, R. G. T. Zegers, B. A. Brown, Sam M. Austin, T. Baugher, D. Bazin, J. Deaven, A. Gade, G. F. Grinyer, C. J. Guess, M. E. Howard, H. Iwasaki, S. McDaniel, K. Meierbachtol, G. Perdikakis, J. Pereira, A. M. Prinke, A. Ratkiewicz, A. Signoracci, S. Stroberg, L. Valdez, P. Voss, K. A. Walsh, D. Weisshaar, and R. Winkler
Phys. Rev. Lett. 108, 122501 – Published 19 March 2012

Abstract

We present a novel technique for studying the quenching of shell gaps in exotic isotopes. The method is based on extracting Gamow-Teller (ΔL=0, ΔS=1) transition strengths [B(GT)] to low-lying states from charge-exchange reactions at intermediate beam energies. These Gamow-Teller strengths are very sensitive to configuration mixing between cross-shell orbitals, and this technique thus provides an important complement to other tools currently used to study cross-shell mixing. This work focuses on the N=8 shell gap. We populated the ground and 2.24 MeV 0+ states in Be12 using the B12(1+) (Li7, Be7) reaction at 80MeV/u in inverse kinematics. Using the ground-state B(GT) value from β-decay measurements (0.184±0.007) as a calibration, the B(GT) for the transition to the second 0+ state was determined to be 0.214±0.051. Comparing the extracted Gamow-Teller strengths with shell-model calculations, it was determined that the wave functions of the first and second 0+ states in Be12 are composed of 25±5% and 60±5% (0s)4(0p)8 configurations, respectively.

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  • Received 18 November 2011

DOI:https://doi.org/10.1103/PhysRevLett.108.122501

© 2012 American Physical Society

Authors & Affiliations

R. Meharchand1,2,3,*, R. G. T. Zegers1,2,3,†, B. A. Brown1,2, Sam M. Austin1,3, T. Baugher1,2, D. Bazin1, J. Deaven1,2,3,‡, A. Gade1,2, G. F. Grinyer1,§, C. J. Guess1,2,3,∥, M. E. Howard3,4,5, H. Iwasaki1,2, S. McDaniel1,2, K. Meierbachtol1,6, G. Perdikakis1,3, J. Pereira1,3, A. M. Prinke1,2,3, A. Ratkiewicz1,2, A. Signoracci1,2,¶, S. Stroberg1,2, L. Valdez1,2,3, P. Voss1,2,**, K. A. Walsh2, D. Weisshaar1, and R. Winkler1,††

  • 1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321, USA
  • 2Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
  • 3Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA
  • 4Department of Physics and Astronomy, Rutgers University, Piscataway, New Jersey 08854, USA
  • 5Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 6Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA

  • *rhiannon.meharchand@gmail.com Present address: Los Alamos National Laboratory, Los Alamos, NM 87545, USA.
  • zegers@nscl.msu.edu
  • Present address: Physics Department, Idaho State University, Pocatello, ID 83209, USA.
  • §Present address: Grand Accélérateur National d’Ions Lourds (GANIL), CEA/DSM-CNRS/IN2P3, Boulevard Henri Becquerel, F-14076 Caen, France.
  • Present address: Department of Physics, University of Massachusetts Lowell, Lowell, MA 01854, USA.
  • Present address: CEA, Centre de Saclay, IRFU/Service de Physique Nucléaire, F-91191 Gif-sur-Yvette, France.
  • **Present address: Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada.
  • ††Present address: Los Alamos National Laboratory, Los Alamos, NM 87545, USA.

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Vol. 108, Iss. 12 — 23 March 2012

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