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We develop a formalism to calculate electromagnetic (EM) transition rates forrotational-vibrational models of nuclei. The formalism is applied to recentlyproposed models of Carbon-12 and Oxygen-16 which are inspired by nucleardynamics in the Skyrme model. We compare the results to experimental data, aswell as other nuclear models. The results for Carbon-12 are in good agreementwith the data across all models, making it difficult to differentiate themodels. More experimental data is needed to do this, and we suggest whichtransitions would be most interesting to measure. The models of Oxygen-16 areless successful in describing the data, and we suggest some possibleimprovements to our approximations which may help.

Electromagnetic transition rates of Carbon-12 and Oxygen-16 in rotational-vibrational models