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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. 12.

Characteristic scales from the amplitude for n = −2. The scaling of characteristic wavenumber scales derived from the departure of the amplitude from linear growth, kc(a, Δc) vs. a is shown for four different values of Δc [see eq. (12) for the definition of kc(a, Δc)]. All the curves have a slope close to the standard self‐similar scaling, kca−2 at high k. For k below about 10, the slope becomes shallower, probably because of the limitation of a finite box.

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