Third-Order Lagrangian Perturbation Theory - Realization at High-Spatial Resolution

Details Third-Order Lagrangian Perturbation Theory - Realization at High-Spatial Resolution Third-Order Lagrangian Perturbation Theory - Realization at High-Spatial Resolution

1993-10-13

arxiv.org/abs/astro-ph/9310022v1

Proc. IAP Colloq. 9 (1993), pp.517-519

Astronomy and Astrophysics

Astrophysics

uuencoded compressed postscript file to appear in: Proc of IAP Colloq. 9, ``Cosmological velocity fields'', ed. F.Bouchet, M.L

Scientific paper

The Lagrangian theory of gravitational instability of homogeneous-isotropic Friedman-Lemaitre cosmogonies investigated and solved in the series of papers by Buchert (1989), (1992), Buchert & Ehlers (1993), Buchert (1993a,b), Ehlers & Buchert (1993), is illustrated. The third-order solution of this theory for generic initial conditions is presented and realized in a special case by employing methods of high-spatial resolution of the density field.

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