Phys. Rev. C 80, 034301 (2009) [9 pages]

²⁶Mg observables for the USDA and USDB Hamiltonians

Abstract

References

Citing Articles (2)

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W. A. Richter¹ and B. Alex Brown²
¹Department of Physics, University of the Western Cape, Private Bag X17, Bellville 7535, South Africa
²Department of Physics and Astronomy, and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321, USA

Received 12 June 2009; published 1 September 2009

Assignments are made between theory and experiment of corresponding levels in ²⁶Mg levels based on energies, lifetimes, branching ratios, electron scattering form factors, and reduced electromagnetic transition strengths. Results based on the new sd-shell interactions USDA (universal sd-shell interaction A) and USDB (universal sd-shell interaction B), as well as the older USD interaction, are compared.

URL:

http://link.aps.org/doi/10.1103/PhysRevC.80.034301

DOI:

10.1103/PhysRevC.80.034301

PACS:

21.10.Ky, 21.10.Jx, 21.60.Cs

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Phys. Rev. C 80, 034301 (2009) [9 pages]

26Mg observables for the USDA and USDB Hamiltonians

²⁶Mg observables for the USDA and USDB Hamiltonians