Results

We are developping the largest cosmological DM simulations to date for realistic DE models with several billion particles and high spatial resolution. Our challenge is to reproduce with unprecedented details the cosmic structure formation process. The goal is to gain a theoretical understanding of the mechanisms that shape the distribution of matter in the universe and which carry an imprint of the nature of Dark Energy. The results will provide a platform of synthetic data to support the next generation of cosmological surveys such as Planck, DES, LSST, Euclid, …

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