On the implementation of the spherical collapse model for dark energy models
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Publication:5021521
DOI10.1088/1475-7516/2017/10/040OpenAlexW3100935764WikidataQ59320347 ScholiaQ59320347MaRDI QIDQ5021521
Sven Meyer, Francesco Pace, Matthias Bartelmann
Publication date: 13 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1708.02477
Related Items (3)
Spherical collapse of non-top-hat profiles in the presence of dark energy with arbitrary sound speed ⋮ Effects of Rastall parameter on perturbation of dark sectors of the Universe ⋮ The growth of DM and DE perturbations in DBI non-canonical scalar field scenario
Uses Software
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