Structure formation refers to a largely unsolved, but extensively researched problem in physical cosmology. The universe, as is now known from observations of the cosmic microwave background radiation, began in a hot, dense, nearly uniform state approximately 13.8 Gyr ago. However, looking in the sky today, we see structures on all scales, from stars and planets to galaxies and, on much larger scales still, galaxy clusters, and enormous voids between galaxies. How did all of this come about from the nearly uniform early universe?
Read more about Structure Formation: Overview, Very Early Universe, Primordial Plasma, Linear Structure, Nonlinear Structure, Gastrophysical Evolution
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