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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. 13.

Characteristic scales from the phase for n = 0. For n = 0 the scaling kc vs. a is shown using the mean phase deviation. Notice that in contrast to the n = −2 case, here only one behavior for all values of φc is evident: the self‐similar scaling kca−2/3.

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