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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. 1.

Power spectrum P(k) vs. k measured from simulation A at five different times. The solid curves show the N‐body power spectrum for knl(a) = 58, 29, 14.5, 7.25. The wavenumber k is in units of 2π/L. The dotted lines show the linear spectrum Pa2k−2 at the same times. The N‐body spectrum at low k shows statistical fluctuations due to the small number of modes available to measure it. At high k the spectrum is plotted up to ﹩\frac{1}{2}﹩ the Nyquist frequency of the FFT grid, k = 512.

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