Simulations of the formation, evolution and clustering of galaxies and quasars

@article{Springel2005SimulationsOT,
  title={Simulations of the formation, evolution and clustering of galaxies and quasars},
  author={Volker Springel and Simon D. M. White and Adrian Jenkins and Carlos S. Frenk and Naoki Yoshida and Liang Gao and Julio F. Navarro and Robert J. Thacker and Darren J. Croton and John C. Helly and John A Peacock and Shaun Cole and Peter A Thomas and Hugh M. P. Couchman and August E. Evrard and J. M. Colberg and Frazer R. Pearce},
  journal={Nature},
  year={2005},
  volume={435},
  pages={629-636}
}
The cold dark matter model has become the leading theoretical picture for the formation of structure in the Universe. This model, together with the theory of cosmic inflation, makes a clear prediction for the initial conditions for structure formation and predicts that structures grow hierarchically through gravitational instability. Testing this model requires that the precise measurements delivered by galaxy surveys can be compared to robust and equally precise theoretical calculations. Here… 
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