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Force Distribution and Relaxation Time in Clusters of Galaxies

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Numerical Astrophysics

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 240))

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Abstract

We examine the influence of nearest neighbor galactic encounters in gravi-tationally clustered systems by using cosmological N-body simulation and determine the two-body relaxation time in the expanding universe, which is based on the effect of two-body encounters in the clusters of galaxies.

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References

  • Aarseth S.J., 1985, Multiple Time Scales Academic Press, New York

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  • Chandrasekhar S., 1942, Principles of Stellar Dynamics, The University of Chicago Press, Chicago

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© 1999 Springer Science+Business Media Dordrecht

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Ardi, E., Tsuchiya, T., Inagaki, S. (1999). Force Distribution and Relaxation Time in Clusters of Galaxies. In: Miyama, S.M., Tomisaka, K., Hanawa, T. (eds) Numerical Astrophysics. Astrophysics and Space Science Library, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4780-4_28

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  • DOI: https://doi.org/10.1007/978-94-011-4780-4_28

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6008-0

  • Online ISBN: 978-94-011-4780-4

  • eBook Packages: Springer Book Archive

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