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In physical cosmology, structure formation describes the creation of galaxies, galaxy clusters, and larger structures via gravitational and hydrodynamic processes operating on cosmological inhomogeneities.: 458 The universe, as is now known from observations of the cosmic microwave background radiation, began in a hot, dense, nearly uniform state…
Dark matter structure, Modelling structure formation & Before the first structures
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universe matter formation dark structure galaxy structures radiation galaxies density gravitational cosmic background larger clusters gauge perturbations form small due
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| the Hubble Ultra-Deep Field | instance of | both via observations | 0.80 | text |
| via large computer simulations | instance of | both via observations | 0.80 | text |
| the first stars | instance of | the smaller gravitationally bound structures | 0.80 | text |
| stellar clusters form | instance of | the smaller gravitationally bound structures | 0.80 | text |
| then galaxies | instance of | the smaller gravitationally bound structures | 0.80 | text |
| followed by groups | instance of | the smaller gravitationally bound structures | 0.80 | text |
| clusters | instance of | the smaller gravitationally bound structures | 0.80 | text |
| superclusters of galaxies.Linear structureDark matter plays a crucial role in structure formation because it feels only the force of gravity | instance of | the smaller gravitationally bound structures | 0.80 | text |
| a star formation | instance of | and the best that can be achieved are approximate simulations that illustrate the main qualitative features of a process | 0.80 | text |
| Structure formation | related to Before the first structures | Structure | 0.60 | section |
| Structure formation | related to Before the first structures | At | 0.60 | section |
| Structure formation | related to Before the first structures | CMB | 0.60 | section |
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