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

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dc.creatorBuchert, T.
dc.creatorWeiss, A. G.
dc.date1993-10-13
dc.date.accessioned2026-07-07T02:18:55Z
dc.date.available2026-07-07T02:18:55Z
dc.descriptionThe 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.
dc.descriptionuuencoded compressed postscript file to appear in: Proc of IAP Colloq. 9, ``Cosmological velocity fields'', ed. F.Bouchet, M.Lachieze-Rey Dummy report number MPA-000-000-93
dc.identifierhttps://arxiv.org/abs/astro-ph/9310022
dc.identifierhttp://arxiv.org/abs/astro-ph/9310022
dc.identifierProc. IAP Colloq. 9 (1993), pp.517-519
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9675
dc.subjectAstrophysics
dc.titleThird-Order Lagrangian Perturbation Theory - Realization at High-Spatial Resolution
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