Millennium Simulation Visualizations

9.11.2014

The cold dark matter model has become the leading theoretical paradigm for the formation of structure in the Universe. Together with the theory of cosmic inflation, this model 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. In the Millennium Simulation project, the Virgo Consortium has presented a novel framework for the quantitative physical interpretation of such surveys. This combines the largest simulation of the growth of dark matter structure carried out up to that time with new techniques for following the formation and evolution of the visible components. In particular, we have shown that baryon-induced features in the initial conditions of the Universe are reflected in distorted form in the low-redshift galaxy distribution, an effect that can be used to constrain the nature of dark energy with next generation surveys.

The Millennium Simulation has also been used to create a number of visualizations of the predicted dark matter structure and the galaxy distribution on large scales, some of them are reproduced on this page. Credit for the visualizations below should be given to V. Springel and the publication:

  • Simulations of the formation, evolution and clustering of galaxies and quasars
    Springel V., White S. D. M., Jenkins A., Frenk C. S., Yoshida N., Gao L., Navarro J., Thacker R., Croton D., Helly J., Peacock J. A., Cole S., et al. (2005)
    Nature, 435, 629 [ADS]
A 3-dimensional visualization of the Millennium Simulation. The movie shows a journey through the simulated universe. On the way, we visit a rich cluster of galaxies and fly around it. During the two minutes of the movie, we travel a distance for which light would need more than 2.4 billion years.

MPEG4, 166 MB, 1920×1080 pixel

This movie shows the dark matter distribution in the universe at the present time, based on the Millennium Simulation, the largest N-body simulation carried out thus far (more than 1010 particles). By zooming in on a massive cluster of galaxies, the movie highlights the morphology of the structure on different scales, and the large dynamic range of the simulation (105 per dimension in 3D). The zoom extends from scales of several Gpc down to resolved substructures as small as ~10 kpc.

divx5, 118 MB, 1024×768 pixel, no annotation

Über das HITS

Das HITS (Heidelberger Institut für Theoretische Studien) wurde 2010 von dem Physiker und SAP-Mitbegründer Klaus Tschira (1940-2015) und der Klaus Tschira Stiftung als privates, gemeinnütziges Forschungsinstitut gegründet. Es betreibt Grundlagenforschung in den Naturwissenschaften, der Mathematik und der Informatik. Zu den Hauptforschungsrichtungen zählen komplexe Simulationen auf verschiedenen Skalen, Datenwissenschaft und -analyse sowie die Entwicklung rechnergestützter Tools für die Forschung. Die Anwendungsfelder reichen von der Molekularbiologie bis zur Astrophysik. Ein wesentliches Merkmal des Instituts ist die Interdisziplinarität, die in zahlreichen gruppen- und disziplinübergreifenden Projekten umgesetzt wird. Die Grundfinanzierung des HITS wird von der Klaus Tschira Stiftung bereitgestellt.

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