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Self‐Similar Evolution of Gravitational Clustering. II. N‐Body Simulations of the n = −2 Spectrum

  • Authors: Bhuvnesh Jain and Edmund Bertschinger

Jain & Bertschinger 1998 The Astrophysical Journal 509 517.

  • Provider: AAS Journals

Caption: Fig. 6.

Identical to Fig. 5 but for simulation B , which has 1283 particles and twice as large a spatial resolution as simulation A. The results shown in the two panels are not able to distinguish the different scalings. This figure demonstrates the need for larger simulations, like the one shown in Figs. 4 and 5, to effectively test the scaling properties of the n = −2 spectrum.

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