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Cosmological model

The Lambda-CDM Model

Cosmology & UniverseStrong Evidence

Definition

The standard model of cosmology: a flat, expanding Universe dominated by a cosmological constant (Λ) and cold dark matter (CDM).

Scientific overview

ΛCDM is the simplest model that fits nearly all cosmological observations — the cosmic microwave background, large-scale structure, the light-element abundances, and the accelerating expansion — with just six parameters. It describes a Universe that is about 68% dark energy, 27% dark matter, and 5% ordinary matter.

Historical development

Emerged in the late 1990s as dark-energy evidence combined with CMB and structure data; refined to percent-level precision by WMAP and Planck.

Evidence

  • Fits the full CMB power spectrum (Planck)
  • Reproduces large-scale structure and BAO
  • Matches Big Bang nucleosynthesis and the accelerating expansion

Parameters

Dark energy (Λ)≈ 68%Planck Collaboration
Cold dark matter≈ 27%Planck Collaboration
Ordinary matter≈ 5%Planck Collaboration
GeometryFlat (Ω ≈ 1)Planck Collaboration

Key ingredients

Open questions

  • What are dark matter and dark energy?
  • Is the Hubble tension a sign of new physics?
  • Is dark energy truly a constant?

Rests on

Knowledge connections

Sources & references

The primary and reference sources this topic draws on.

  • Planck CollaborationESA Planck mission / Planck Collaboration

    Cosmic microwave background maps and the cosmological parameters of the ΛCDM model.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.