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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. 3.

Effect of limited resolution on the power spectrum. The solid curves show the power spectrum measured from simulation C, a PM simulation with the same number of particles as simulation A, a P3M simulation. The spectra are computed on a 5123 grid and are shown at the same output times as those of Figure 1. The dotted curves show the spectra from simulation A, computed using a 10243 grid. Both spectra are plotted up to ﹩\frac{1}{2}﹩ the Nyquist frequency of the FFT grid. A comparison of the two sets of spectra shows that as time evolves, the power in the PM simulation is suppressed on an increasingly large range of k.

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