Abstract
We have computed matter radii for the ground states of ${}^{29--35}$Mg for a variety of reasonable assumptions about the structure of the relevant states. For cases in which the dominant configuration is generally agreed, our computed radii are in good agreement with experimental ones. For cases in which the dominant configuration is unknown or ambiguous, comparisons between the calculated and experimental ${R}_{m}$ do not allow a decision as to the preferred configuration.
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