A viscous interacting dark-energy model is fitted to Type Ia supernovae and is claimed, via linear perturbations, to predict the disintegration of large-scale bound structures at late times.
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Viscous cosmological fluids and large-scale structure
A viscous interacting dark-energy model is fitted to Type Ia supernovae and is claimed, via linear perturbations, to predict the disintegration of large-scale bound structures at late times.