Spherical collapse of non-top-hat profiles in the presence of dark energy with arbitrary sound speed

DOI10.1088/1475-7516/2023/02/037OpenAlexW4320917088MaRDI QIDQ5882752

R. C. Batista, H. P. de Oliveira, L. Raul W. Abramo

Publication date: 17 March 2023

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2210.14769

zbMATH Keywords

dark energy theorygalaxy clusterscluster counts

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Cites Work

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• The imperfect fluid behind kinetic gravity braiding
• On the spherical collapse model in dark energy cosmologies
• On the implementation of the spherical collapse model for dark energy models
• Dark energy perturbations in N-body simulations
• k-evolution: a relativistic N-body code for clustering dark energy

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