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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. 10.

Amplitude trajectories for n = −2. The trajectories of the amplitudes Δ(k, τ) of individual Fourier modes for n = −2 are plotted vs. a, as in Fig. 9 for the phase. Note that at early times Δ ∝ a: to check this, all the curves have been joined to Δ = 0 at a = 0. Therefore the lowest value of a at which departures from a straight line occur shows nonlinear behavior.

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