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Nonlinear evolution of spherical perturbation in a non-flat Universe with cosmological constant

2001/08/17 by Ewa L. Lokas, Yehuda Hoffman, Lokas, Ewa L. +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0108283

7 pages, 5 figures, results for quintessence removed (as obtained with an unjustified assumption of the conservation of energy inside the overdense region)

arxiv created 2002/07/25 · arxiv updated 2009/12/01

Abstract

We generalize the spherical collapse model for the formation of bound objects to apply in a Universe with arbitrary positive cosmological constant. We calculate the critical condition for collapse of an overdense region and give exact values of the characteristic densities and redshifts of its evolution.

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