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arxiv: gr-qc/0106096 · v2 · submitted 2001-06-29 · 🌀 gr-qc · astro-ph

Structure formation in the Lemaitre-Tolman model

classification 🌀 gr-qc astro-ph
keywords lemaitre-tolmanmodelstructuredensityevolutionformationinvestigatedmass
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Structure formation within the Lemaitre-Tolman model is investigated in a general manner. We seek models such that the initial density perturbation within a homogeneous background has a smaller mass than the structure into which it will develop, and the perturbation then accretes more mass during evolution. This is a generalisation of the approach taken by Bonnor in 1956. It is proved that any two spherically symmetric density profiles specified on any two constant time slices can be joined by a Lemaitre-Tolman evolution, and exact implicit formulae for the arbitrary functions that determine the resulting L-T model are obtained. Examples of the process are investigated numerically.

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