Hydrodynamical adaptive mesh refinement simulations of turbulent flows-II . Cosmological simulations of galaxy clusters

@inproceedings{Iapichino2008HydrodynamicalAM,
  title={Hydrodynamical adaptive mesh refinement simulations of turbulent flows-II . Cosmological simulations of galaxy clusters},
  author={Laura Iapichino and Jens C. Niemeyer},
  year={2008}
}
The development of turbulent gas flows in the intra-cluster medium and in the core of a galaxy cluster is studied by means of adaptive mesh refinement (AMR) cosmological simulations. A series of six runs was performed, employing identical simulation parameters but different criteria for triggering the mesh refinement. In particular, two different AMR strategies were followed, based on the regional variability of control variables of the flow and on the overdensity of subclumps, respectively. We… CONTINUE READING

Citations

Publications citing this paper.

References

Publications referenced by this paper.
Showing 1-3 of 3 references

Large Eddy Simulation for Incompressible Flows. An Introduction

  • P. Sagaut
  • 2001
1 Excerpt

Physics of Fully Ionized Gases

  • L. Spitzer
  • New York: Interscience (2nd edition),
  • 1962
2 Excerpts

Similar Papers

Loading similar papers…