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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References

SHOWING 1-10 OF 133 REFERENCES
A recipe for galaxy formation
We present a detailed prescription for how galaxy formation can be modelled in hierarchical theories of structure formation. Our model incorporates the formation and merging of dark matter halos, the
The evolution of large-scale structure in a universe dominated by cold dark matter
The results of numerical simulations of nonlinear gravitational clustering in universes dominated by weakly interacting, 'cold' dark matter are presented. The numerical methods used and the way in
The Epoch of Galaxy Formation
We use a semianalytic model of galaxy formation in hierarchical clustering theories to interpret recent data on galaxy formation and evolution, focusing primarily on the recently discovered
A unified model for the evolution of galaxies and quasars
We incorporate a simple scheme for the growth of supermassive black holes into semi-analytic models that follow the formation and evolution of galaxies in a cold dark matter-dominated Universe. We
Clustering of galaxies in a hierarchical universe - I. Methods and results at z=0
We introduce a new technique for following the formation and evolution of galaxies in cosmological N-body simulations. Dissipationless simulations are used to track the formation and merging of dark
Populating a cluster of galaxies - I. Results at z=0
ABSTRA C T We simulate the assembly of a massive rich cluster and the formation of its constituent galaxies in a flat, low-density universe. Our most accurate model follows the collapse, the star
The nature of galaxy bias and clustering
We have used a combination of high resolution cosmological N-body simulations and semi-analytic modelling of galaxy formation to investigate the processes that determine the spatial distribution of
Mergers and bias in a cold dark matter cosmology
A dissipative N-body code is used to follow the evolution of a cold dark matter spectrum in an Omega = 1, h = 0.5 background. The star and galaxy formation in boxes of three different sizes is shown,
How filaments of galaxies are woven into the cosmic web
LARGE-SCALE structure in the distribution of galaxies is thought to have evolved through gravitational instabilities from small density fluctuations in the (largely homogeneous) early Universe. This
The formation and evolution of galaxies within merging dark matter haloes
We construct semi-analytic models for galaxy formation within the framework of a hierarchical clustering scenario for structure formation in the Universe. We use the algorithm of Kauffmann & White to
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