Non-linear structure formation in cosmologies with early dark energy

DOI10.1051/0004-6361:20053922zbMath1134.85309arXivastro-ph/0507257OpenAlexW2026200686WikidataQ56937410 ScholiaQ56937410MaRDI QIDQ3408425

M. Doran, Christof Wetterich, Matthias Bartelmann

Publication date: 1 November 2006

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0507257

zbMATH Keywords

early Universelarge-scale structure of Universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Astrophysical cosmology (85A40)

Related Items (3)

THE INFLUENCE OF DARK ENERGY ON THE LARGE SCALE STRUCTURE FORMATION ⋮ Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant ⋮ On the implementation of the spherical collapse model for dark energy models

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