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Merging Rate of Dark Matter Halos: Evolution and Dependence on Environment

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Abstract

We discuss the impact of the cosmological environment on the evolution of dark matter halos using a high-resolution simulation within a spatially flat ACDM cosmology.

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References

  • Avila-Reese, V., Firmani, C., Klypin, A. and Kravtsov, A.V.: 1999, Density profiles of dark matter haloes: diversity and dependence on environment, Mon. Not. R. Astron. Soc., 310, 527–539.

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  • Gottlöber, S., Klypin, A.A. and Kravtsov, A.V.: 1999, Halo evolution in a cosmological environment, in: G. Giuricin, M. Mezetti and P. Saluccip (eds.), Observational Cosmology: The Development of Galaxy Systems, ASP Conference Series 176, 418–429.

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  • Klypin, A.A., Gottlöber, S., Kravtsov, A.V. and Khokhlov. A.M.: 1999, Galaxies in N-body Simulations: Overcoming the Overmerging Problem, Astrophys. J. 516, 530–551.

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  • Kravtsov, A.V., Klypin, A.A. and Khokhlov, A.M.: 1997, Adaptive Refinement Tree: A new high-resolution N-body code for cosmological simulations, Astrophys. J. Suppl. See 111, 73–94.

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© 2000 Springer Science+Business Media Dordrecht

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Gottlöber, S., Klypin, A., Kravtsov, A.V. (2000). Merging Rate of Dark Matter Halos: Evolution and Dependence on Environment. In: Block, D.L., Puerari, I., Stockton, A., Ferreira, D. (eds) Toward a New Millennium in Galaxy Morphology. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4114-7_25

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  • DOI: https://doi.org/10.1007/978-94-011-4114-7_25

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-5801-8

  • Online ISBN: 978-94-011-4114-7

  • eBook Packages: Springer Book Archive

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