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Spherical collapse of dark matter haloes in tidal gravitational fields

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We study the spherical collapse model in the presence of external gravitational tidal shear fields for different dark energy scenarios and investigate the impact on the mass function and cluster number counts. While previous studies of the influence of shear and rotation on δc have been performed wi...

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Main Authors: Reischke, Robert (Author) , Pace, Francesco (Author) , Meyer, Sven (Author) , Schäfer, Björn Malte (Author)
Format: Article (Journal)
Language:English
Published: 10 August 2016
In: Monthly notices of the Royal Astronomical Society
Year: 2016, Volume: 463, Issue: 1, Pages: 429-440
ISSN:1365-2966
DOI:10.1093/mnras/stw1989
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw1989
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/463/1/429/2589852
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Author Notes:Robert Reischke, Francesco Pace, Sven Meyer, Björn Malte Schäfer
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Spherical collapse of dark matter haloes in tidal gravitational fields by Reischke, Robert (Author) , Pace, Francesco (Author) , Schäfer, Björn Malte (Author) ,


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