Abstract
An energy-weighted sum rule for magnetic multipole transitions $M\ensuremath{\lambda}$ is proposed as a generalization of the Kurath sum rule. The role of the spin-orbit potential is discussed, and corrections due to nuclear interaction are calculated explicitly using Skyrme forces. It is shown that, while for $\ensuremath{\lambda}=1$ the whole contribution comes from spin-orbit potential, for $\ensuremath{\lambda}g1$ the main part is due to the kinetic energy.
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