FLRW cosmological models

E1311

FLRW cosmological models are a family of solutions to Einstein’s field equations that describe a homogeneous and isotropic expanding or contracting universe, forming the standard framework for modern cosmology.

All labels observed (17)

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Statements (51)

Predicate Object
instanceOf cosmological model
homogeneous cosmological model
isotropic cosmological model
solution to Einstein field equations
spacetime metric
spacetime metric
allowsSpatialCurvature negative curvature
positive curvature
zero curvature
approximates large-scale structure of the universe
assumes cosmological principle
large-scale homogeneity
large-scale isotropy
basedOnTheory general relativity
compatibleWith cosmic microwave background isotropy
definedOn four-dimensional spacetime
describes contracting universe
expanding universe
homogeneous universe
isotropic universe
fullName FLRW cosmological models self-linksurface differs
surface form: Friedmann–Lemaître–Robertson–Walker cosmological models
governedBy Einstein field equations
surface form: Friedmann equations
hasLimitation assumes perfect fluid description of matter
neglects small-scale inhomogeneities
hasMetric FLRW cosmological models self-linksurface differs
surface form: FLRW metric
historicalDevelopment first solutions found by Alexander Friedmann in the 1920s
general form clarified by Robertson and Walker in the 1930s
implies Hubble–Lemaître law on large scales
includes cosmic time coordinate
scale factor
spatial curvature parameter
includesComponent baryonic matter
dark energy
dark matter
radiation
includesParameter cosmological constant
namedAfter Alexander Friedmann
Arthur Geoffrey Walker
Georges Lemaître
Howard P. Robertson
predicts cosmic expansion history
time-dependent scale factor
spatialSections 3-sphere
Euclidean 3-space
hyperbolic 3-space
usedIn standard model of cosmology
ΛCDM model
usedToInfer age of the universe
cosmological distance–redshift relations
critical density of the universe
validAtScale cosmological scales

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Referenced by (37)

Full triples — surface form annotated when it differs from this entity's canonical label.

Oppenheimer–Snyder model usesMetric FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Oppenheimer–Snyder model relatedTo FLRW cosmological models
FLRW cosmological models fullName FLRW cosmological models self-linksurface differs
this entity surface form: Friedmann–Lemaître–Robertson–Walker cosmological models
FLRW cosmological models hasMetric FLRW cosmological models self-linksurface differs
this entity surface form: FLRW metric
Einstein field equations admitsSolution FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
de Sitter spacetime hasMetricType FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric (special case)
Arthur Geoffrey Walker notableWork FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Arthur Geoffrey Walker notableWork FLRW cosmological models
this entity surface form: Robertson–Walker metric
Arthur Geoffrey Walker notableConcept FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker cosmological model
Alexander Friedmann knownFor FLRW cosmological models
this entity surface form: Friedmann equations
Howard P. Robertson notableWork FLRW cosmological models
this entity surface form: Robertson–Walker metric
Howard P. Robertson notableWork FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Howard P. Robertson notableWork FLRW cosmological models
this entity surface form: Robertson–Walker cosmological models
general relativity includes FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Big Bang basedOn FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Penrose–Carter diagrams appliesTo FLRW cosmological models
subject surface form: Penrose–Carter diagram
this entity surface form: Friedmann–Lemaître–Robertson–Walker cosmologies
On the Curvature of Space proposedModel FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
On the Curvature of Space proposedModel FLRW cosmological models
this entity surface form: Friedmann cosmological models
Big Bang cosmology basedOn FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
hypothesis of the primeval atom associatedWith FLRW cosmological models
this entity surface form: Lemaître’s expanding universe solution
Lemaître–Hubble law relatedTo FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Lemaître–Hubble law relatedTo FLRW cosmological models
this entity surface form: Friedmann equations
Gödel metric contrastsWith FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Lemaître–Tolman metric generalizes FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Lambda-CDM model basedOn FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Gravitation (with Charles Misner and Kip Thorne) covers FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker cosmological models
Tolman surface brightness test basedOn FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Gravitation and Cosmology subject FLRW cosmological models
this entity surface form: Friedmann–Robertson–Walker cosmology
Planck temperature usedIn FLRW cosmological models
this entity surface form: Big Bang models
American school of relativistic cosmology relatedTo FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Bardeen potential appliesTo FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Principles of Physical Cosmology topic FLRW cosmological models
this entity surface form: Friedmann–Robertson–Walker models
Weyl tensor vanishesIn FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker spacetimes
Rubin–Ford effect cosmologicalContext FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker cosmology
Einstein static universe relatedTo FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker metric
Einstein static universe specialCaseOf FLRW cosmological models
chaotic inflation mathematicalFramework FLRW cosmological models
this entity surface form: Friedmann–Lemaître–Robertson–Walker cosmology