C. E. Pellicer, Elisa G. M. Ferreira, Daniel C. Guariento, André A. Costa, Leila L. Graef, Andrea Coelho, Elcio Abdalla
We consider a toy model to analyze the consequences of dark matter interaction with a dark energy background on the overall rotation of galaxy clusters and the misalignment between their dark matter and baryon distributions when compared to {\Lambda}CDM predictions. The interaction parameters are found via a genetic algorithm search. The results obtained suggest that interaction is a basic phenomenon whose effects are detectable even in simple models of galactic dynamics.
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http://arxiv.org/abs/1102.5113
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