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Observation of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>C</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>46</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow><mml:mi>r</mml:mi></mml:math>and Testing the Isobaric Multiplet Mass Equation at High Spin

P. E. GarrettLawrence Livermore National Laboratory, Livermore, California 94551, USAW. E. OrmandLawrence Livermore National Laboratory, Livermore, California 94551D. E. AppelbeDepartment of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, CanadaRoman BauerLawrence Livermore National Laboratory, Livermore, California 94551J. A. BeckerLawrence Livermore National Laboratory, Livermore, California 94551L. A. BernsteinLawrence Livermore National Laboratory, Livermore, California 94551J. A. CameronDepartment of Physics and Astronomy, McMaster University, Hamilton, Ontario L8S 4M1, CanadaM. P. CarpenterPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439R. V. F. JanssensPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439C. J. ListerPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439D. SeweryniakPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439E. TavukcuNorth Carolina State University, Raleigh, North Carolina 27695D. D. WarnerCLRC Daresbury Laboratory, Daresbury, Warrington, WA4 4AD, United Kingdom
2001lv
ABI

Аннотация

The ground state band in ${}^{46}\mathrm{Cr}$ and the isospin $T\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}1$ band in ${}^{46}\mathrm{V}$ have been delineated up to ${I}^{\ensuremath{\pi}}{\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}10}^{+}$ (tentatively ${12}^{+}$). These observations complete the highest spin $T\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}1$ isospin triplet known. Following the isobaric multiplet mass equation, a combination of level energies in ${}^{46}\mathrm{Cr}$, ${}^{46}\mathrm{Ti}$, and ${}^{46}\mathrm{V}$ are taken to highlight the angular momentum dependence of the isovector and isotensor parts of the interaction. The results are compared with full- $\mathrm{fp}$-space shell model calculations. The influence of the one-body and two-body contributions to the isovector energy difference are investigated.

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