Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations

The top-hat spherical collapse model (TSC) is one of the most fundamental analytical frameworks to describe the non-linear growth of cosmic structure. TSC has motivated, and been widely applied in, various researches even in the current era of precision cosmology. While numerous studies exist to exa...

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Veröffentlicht in:	arXiv.org 2015-11
Hauptverfasser:	Suto, Daichi, Kitayama, Tetsu, Osato, Ken, Sasaki, Shin, Suto, Yasushi
Format:	Artikel
Sprache:	eng
Schlagworte:	Collapse Computer simulation Cosmology Dark matter Density Dynamical systems Galactic halos Inhomogeneity Mathematical models Nonuniformity Physics - Cosmology and Nongalactic Astrophysics
Online-Zugang:	Volltext
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