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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. 9.

"Redefined" phase trajectories for n = −2. The same trajectories as in Fig. 8 are plotted, but φ has been redefined so that it is no longer constrained between −π and π (notice the limits on the y‐axis), as described in § 5.1. In linear theory the phases do not change with time; significant departures from this can be seen in all but the lowest k modes.

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