Dark energy and the evolution of spherical overdensities

Astronomy and Astrophysics – Astrophysics

Scientific paper

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9 pages, 8 figures. Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2005.09140.x

We use the non-linear spherical model in cold dark matter (CDM) cosmologies with dark energy to investigate the effects of dark energy on the growth of structure and the formation of virialised structures. We consider dark energy models with a constant equation of state parameter w. For -1

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