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On Local Approximations to the Nonlinear Evolution of Large‐Scale Structure

  • Authors: Martín Makler, Takeshi Kodama, and Maurício O. Calvão

Makler, Kodama, & Calvão 2001 The Astrophysical Journal 557 88.

  • Provider: AAS Journals

Caption: Fig. 1.

Evolution of the three axes Ri of an ellipsoid according to the homogeneously collapsing ellipsoid model (HCE; solid curve), and the five approximations considered in the text: Zeldovich (ZA; dotted curve), modified Zeldovich (MZA; short‐dotted curve), deformation tensor (DTA; dot‐dashed curve), complete Zeldovich (CZA; short‐dashed curve), and local tidal (LTA; long‐dashed curve). The initial axis ratios are 1:1.25:1.5, and the density contrast linearly extrapolated to ﹩a=1﹩ is ﹩\delta _{0}=1﹩. The ZA overestimates the collapse time, whereas all other approximations are close to the HCE.

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