Magnetic moments of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msubsup><mml:mn>2</mml:mn><mml:mrow><mml:mn>1</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math>states around<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Sn</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>132</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>
B. A. BrownDepartment of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USAN. J. StoneDepartment of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USAJ. R. StoneDepartment of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USAI. S. TownerPhysics Department, Queen's University, Kingston, Ontario, Canada K7L 3N6M. Hjorth‐JensenDepartment of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
2005lv
ABI
Аннотация
Development of neutron-rich radioactive beams at the Holifield Radioactive Ion Beam Facility has stimulated experimental and theoretical activity in heavy Sn and Te isotopes. Recently, the g factor of the first ${2}^{+}$ state in $^{132}\mathrm{Te}$ has been measured. We report here new shell-model calculation of magnetic moments for selected Sn and Te isotopes. The residual interaction is based on the CD-Bonn renormalized $G$ matrix. Single-particle spin and orbital effective g factors are evaluated microscopically including core polarization and meson exchange currents effects.
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