The Standard Cosmological Model - also called Lambda-CDM (ΛCDM), where Λ denotes the cosmological constant and CDM stands for cold dark matter - is the prevailing scientific framework describing the large-scale structure, composition, and evolution of the universe. It posits that the universe originated in a hot, dense state approximately 13.8 billion years ago (an event commonly called the Big Bang), has been expanding ever since, and is presently composed of roughly 5% ordinary (baryonic) matter, 27% cold dark matter, and 68% dark energy, the latter represented by the cosmological constant. The model rests on General Relativity as its gravitational foundation, supplemented by quantum field theory, and is calibrated against observations including the cosmic microwave background (CMB), the large-scale distribution of galaxies, and the luminosity-distance relationship of Type Ia supernovae.

ΛCDM describes a spatially flat universe whose expansion is governed by the Friedmann equations, derived from General Relativity applied to a homogeneous, isotropic spacetime (the cosmological principle). Its major physical components are:

• Baryonic matter - ordinary matter made of protons, neutrons, and electrons, comprising stars, gas, dust, and planets.
• Cold dark matter (CDM) - a hypothetical non-baryonic component that interacts gravitationally but does not emit, absorb, or reflect light. Its existence is inferred from galactic rotation curves, gravitational lensing, and large-scale structure formation.
• Dark energy (Λ) - a term in Einstein's field equations acting as a repulsive energy density uniformly distributed through space, held responsible for the observed accelerating expansion of the universe first measured in 1998 via supernova surveys.¹⁾
• Cosmic inflation - a hypothesized epoch of exponential expansion in the first fraction of a second after the Big Bang, introduced to explain the flatness of spacetime geometry, the uniformity of the CMB, and the absence of magnetic monopoles. Inflation remains unconfirmed at the observational level and is not strictly part of ΛCDM, but is widely incorporated into the standard picture.

The CMB - relic thermal radiation from approximately 380,000 years after the Big Bang, first detected by Penzias and Wilson in 1965 and mapped in detail by the COBE, WMAP, and Planck satellite missions - provides the primary empirical anchor for ΛCDM parameter estimates.²⁾

ΛCDM achieves excellent agreement with a wide range of cosmological observations and is the basis for the great majority of contemporary cosmological research. Several tensions and unresolved questions, however, are subjects of active investigation and, in some cases, scientific controversy:

• The Hubble tension - measurements of the current expansion rate (the Hubble constant, H0) derived from the early universe (CMB) and from late-universe distance ladders (Cepheid variables, supernovae) differ by several standard deviations, a discrepancy that has sharpened as measurement precision has improved.³⁾ Whether this reflects systematic measurement error, a fundamental flaw in ΛCDM, or new physics remains unresolved.
• The S8 tension - independent measurements of the amplitude of matter clustering show a similar, though less severe, discrepancy between early- and late-universe probes.
• The nature of dark matter and dark energy - neither has been directly detected or identified with a known particle or field. The cosmological constant interpretation of dark energy is consistent with data but lacks a satisfactory physical explanation; the predicted vacuum energy density from quantum field theory differs from the observed value by many orders of magnitude (the cosmological constant problem).
• The origin of baryon asymmetry - ΛCDM does not explain why the universe contains substantially more matter than antimatter.
• Alternatives to inflation - bounce cosmologies, string gas cosmology, and other frameworks propose different mechanisms for the early universe's initial conditions.

Some researchers argue the accumulating tensions warrant consideration of extensions or replacements to ΛCDM, while others maintain the model is robust and the tensions reflect uncharacterized systematics in observations.

Strong consensus exists within the physics and astronomy communities that ΛCDM provides the best currently available description of the universe's large-scale structure and evolution. See Cosmology - Physics Consensus for a characterization of that consensus and its scope. Consensus on the model's foundations does not extend to the physical identity of dark matter or dark energy, the correct resolution of the Hubble tension, or the precise mechanism of early-universe inflation.

• ΛCDM as Established Framework - The view that ΛCDM, despite open questions, is sufficiently confirmed by independent lines of evidence to serve as the working standard model, analogous to the Standard Model of particle physics.
• Modified Gravity Alternatives - The view that discrepancies such as galactic rotation curves and the Hubble tension are better explained by modifications to General Relativity (e.g., MOND, MOG, or relativistic extensions) rather than by invoking undetected dark matter and dark energy.
• Plasma Cosmology - A minority view holding that electromagnetic forces operating on cosmic plasma, rather than gravity alone and the Big Bang framework, can account for large-scale structure without dark matter or dark energy.
• Steady State and Eternal Universe Models - Historical and contemporary views that reject a singular origin event in favor of a universe without a definite beginning, including Hoyle's original steady-state model and later variants such as eternal inflation or cyclic cosmologies.
• Crisis in Cosmology - The view held by a minority of working cosmologists that the accumulation of tensions (Hubble, S8, and others) indicates ΛCDM is approaching falsification and requires fundamental revision, not merely parameter adjustment.

• Standard Cosmological Model - History
• Standard Cosmological Model - Debate
• Cosmology - Physics Consensus
• General Relativity
• Big Bang
• Cosmological Constant Problem
• Dark Matter
• Dark Energy
• Cosmic Inflation
• Hubble Tension