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The 53 pages that link to Lambda-CDM model, each with the reason it gives.

• Cosmic microwave backgroundRelated: Its parameters are tightly constrained by the background’s measured patterns.

• Cosmological constantRelated: Its lambda is the constant used to account for late-time accelerated expansion.

• Galaxy mergerRelated: Its predictions for structure growth make galaxy merging a routine part of cosmic evolution.

• CosmologyRelated: It is the benchmark framework that organizes much of modern cosmology's evidence.

• Hubble tensionRelated: Extrapolating this model from the cosmic microwave background predicts a lower Hubble constant.

• Friedmann equationsBroader topic: Its expansion history is calculated by solving the Friedmann equations for these components.

• Local GroupNarrower topic: It describes how the Local Group assembled within a universe dominated by dark matter and accelerated expansion.

• Large-scale structure of the universeNarrower topic: It is the baseline model whose predictions are tested against observed structure.

• Steady-state theoryCompared with: It explains cosmic expansion and observations without continuous creation maintaining constant density.

• Cosmological constant problemRelated: It fits a wide range of observations while leaving the constant’s tiny value unexplained.

• Hierarchical structure formationNarrower topic: It provides the background expansion and matter content for hierarchical growth.

• Modified Newtonian dynamicsCompared with: It fits cosmological observations that basic MOND does not address by itself.

• Planck satelliteRelated: Planck’s measurements tightly constrained this model’s parameters and supported its six-parameter form.

• Galaxy groupNarrower topic: It predicts the dark-matter framework in which galaxy groups form and grow.

• Cold dark matterRelated: It uses cold dark matter to explain structure growth and observations of the universe.

• Roger PenroseCompared with: Penrose’s conformal cyclic cosmology departs from this standard account of the universe’s large-scale history.

• Age of the universeRelated: Its fitted expansion history gives the standard age estimate.

• Accelerating expansion of the universeRelated: It incorporates accelerated expansion through its cosmological-constant component.

• Bullet ClusterRelated: The cluster’s displaced mass fits the model’s picture of weakly interacting dark matter.

• Cosmic microwave background anisotropyRelated: Its parameters are tightly constrained by the observed anisotropy patterns.

• Sloan Great WallRelated: The wall’s abundance and scale can be compared with structure formation predicted by this model.

• Wilkinson Microwave Anisotropy ProbeRelated: WMAP’s parameter measurements strongly supported this model of cosmic evolution.

• Cosmological parametersBroader topic: It gives cosmological parameters a specific, widely tested model context.

• Modified gravityCompared with: It explains cosmic acceleration and structure using dark components rather than altered gravitational laws.

• Tidal dwarf galaxyRelated: Its standard account builds galaxies inside dark-matter halos, unlike tidal-dwarf formation.

• Big CrunchCompared with: Its measured expansion history favors continued acceleration, not an imminent Big Crunch.

• Brian SchmidtRelated: The accelerating expansion became a defining observation the model must explain.

• Dark Energy SurveyRelated: DES tested this model’s predictions for expansion and structure growth.

• High-Z Supernova Search TeamRelated: The supernova evidence helped establish accelerated expansion as a central feature of this model.

• Saul PerlmutterRelated: Its cosmological-constant component accounts for the acceleration established by the supernova result.

• Supernova Cosmology ProjectRelated: The project’s result helped make a cosmological constant central to the standard model.

• Vera RubinRelated: Rubin’s observations helped make dark matter a foundational ingredient of cosmology.

• Local VoidRelated: Its predictions provide a framework for comparing the Local Void with simulated cosmic structure.

• Missing baryon problemNarrower topic: Its early-universe parameters predict the total baryon budget used in the discrepancy.

• Cyclic modelCompared with: Its successful account of observations describes expansion without requiring recurring cycles.

• De Sitter universeRelated: Its far-future expansion approaches De Sitter behavior if the cosmological constant remains constant.

• BOSS Great WallRelated: Simulations based on this model provide a framework for comparing observed structures with cosmic growth.

• Cosmic Background ExplorerNarrower topic: COBE’s primordial fluctuation measurements helped establish the model’s observational basis.

• John C. MatherRelated: COBE’s anisotropy measurements helped make precision tests of this model possible.

• Physical cosmologyRelated: It is the leading framework against which cosmological observations are interpreted.

• Boötes VoidRelated: It predicts the growth and distribution of large cosmic voids such as this one.

• CMB cold spotCompared with: The spot’s statistical unusualness is assessed against predictions of this model.

• Galactic astronomyRelated: It predicts that the Milky Way assembled through growth and mergers within a dark matter halo.

• Galaxy rotation problemRelated: It places galaxy rotation curves within a broader model of cosmic structure and dark matter.

• Huge-LQGRelated: Its predictions provide a baseline for judging whether structures like Huge-LQG are unexpected.

• Observational cosmologyRelated: It provides the baseline predictions that observations test.

• Dark flowCompared with: Its expected large-scale flows provide a benchmark for evaluating dark flow.

• Jim PeeblesBroader topic: This specific model embodies many theoretical ideas Peebles helped develop, though its ingredients remain debated.

• List of unsolved problems in physicsRelated: Its predictive successes coexist with unresolved questions about dark matter and dark energy.

• Local HoleCompared with: Its predicted density fluctuations provide the baseline against which the Local Hole is assessed.