= Spherical Collapse Model
{wiki=Spherical_Collapse_Model}
The Spherical Collapse Model is a theoretical framework used in cosmology to understand the formation of structure in the universe, particularly galaxies and galaxy clusters. It provides a simplified way to study how density perturbations evolve under the influence of gravitational collapse. \#\#\# Key Features of the Spherical Collapse Model: 1. **Initial Conditions**: - The model starts with an initial density perturbation, often assumed to be spherically symmetric.
Back to article page
