| Display title | Astronomy:Cosmological perturbation theory |
| Default sort key | Cosmological Perturbation Theory |
| Page length (in bytes) | 15,724 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374476 |
| Page content language | en - English |
| Page content model | wikitext |
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| Counted as a content page | Yes |
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| Page creator | imported>LinuxGuru |
| Date of page creation | 12:18, 6 February 2024 |
| Latest editor | imported>LinuxGuru |
| Date of latest edit | 12:18, 6 February 2024 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | In physical cosmology, cosmological perturbation theory is the theory by which the evolution of structure is understood in the Big Bang model. Cosmological perturbation theory may be broken into two categories: Newtonian or general relativistic. Each case uses its governing equations to compute gravitational... |
