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M. Brockamp, H. Baumgardt and P. Kroupa, “Tidal Dis-ruption Rate of Stars by Supermassive Black Holes Ob-tained by Direct N-Body Simulations,” arXiv: 1108.2270v1, 2011.

has been cited by the following article:

• TITLE: Numerical Investigations of a New N-body Simulation Method

  AUTHORS: E. Vilkoviskij

  KEYWORDS: N-Body Simulations; Numerical Methods

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.2 No.3, September 28, 2012

  ABSTRACT: Numerical investigation of a new similarity method (the Aldar-Kose method) for N-body simulations is described. Using this method we have carried out numerical simulations for two tasks: 1) calculation of the temporal behavior of different physical parameters of active galactic nuclei (AGN) containing a super massive black hole (SMBH), an accretion disk, and a compact stellar cluster; 2) calculation of the stellar capture rate to the central SMBH without accretion disk. The calculations show good perspectives for applications of the similarity method to optimize the evolution model calculations of large stellar systems and of AGN.