Cosmic structure growth and dark-matter modelling
In the standard cosmological model, small density variations grow gravitationally and dark-matter structures help concentrate baryonic matter after photon coupling becomes less effective.
Key knowledge
In the standard cosmological model, small density variations grow gravitationally and dark-matter structures help concentrate baryonic matter after photon coupling becomes less effective. Gas cooling, star formation, feedback and mergers then affect the luminous galaxies. Observed clustering tests this account alongside the CMB and expansion evidence.
Conditions and scope
- Cold dark matter and the adopted expansion history are model assumptions; dark matter's microscopic identity remains unresolved.
- This qualitative account is not a calculated growth function or a complete nonlinear galaxy-formation model.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Read dark-matter gravitational-trap and later assembly paragraphs; replaced the source's absolute 'does not interact with photons at all' with the standard model's effectively weak photon coupling, and omitted dated earliest-galaxy ages.
2026-10-10 · Independent AI editorial review: All26 Life-authored Cosmos compact statements, conditions, displayed equations and all56 origin semantic links read. Entire26-entry author statement/source matrix and explicit exclusions assessed. Targeted independent primary sections are listed below; this does not claim every referenced source body or proof was independently re-read. This is scoped AI reference-content review, not human disciplinary certification or whole-field completion. Receipt: cosmos-life-independent-content-review.1.
Entry details
Permanent link to this entry ↗- Record identity
- uni-cosmos-structure-growth
- Revision
- core.1
- Structured reference record
- University core expansion