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We present the results of the first N-body simulations of the GrowingNeutrino scenario, as recently discussed in Baldi et al. (2011). Our resultshave shown for the first time how neutrino lumps forming in the context ofGrowing Neutrino cosmologies are expected to pulsate as a consequence of therapid oscillations of the dark energy scalar field. We have also computed forthe first time a realistic statistical distribution of neutrino halos anddetermined their impact on the underlying Cold Dark Matter structures.

The nonlinear evolution of large scale structures in Growing Neutrino cosmologies