Einstein field equations

E1603

The Einstein field equations are the core mathematical framework of general relativity, relating the curvature of spacetime to the distribution of matter and energy.

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Predicate Object
instanceOf equations of general relativity
fundamental physical law
system of equations
tensor equation
admitsSolution FLRW cosmological models
surface form: Friedmann–Lemaître–Robertson–Walker metric

Kerr metric
Minkowski space-time
surface form: Minkowski spacetime

Reissner–Nordström metric
Schwarzschild black hole
surface form: Schwarzschild metric

de Sitter spacetime
basedOnPrinciple equivalence principle
general covariance
constant Newtonian gravitational constant G
cosmological constant \Lambda
speed of light c
contrastsWith quantum gravity theories
describes relationship between spacetime curvature and energy-momentum
difficulty analytical solutions are rare
domain classical gravitation
field general relativity
foundationOf modern cosmology
hasVacuumForm G_{\mu\nu} + \Lambda g_{\mu\nu} = 0
R_{\mu\nu} = 0 (for \Lambda = 0 and vacuum)
includes cosmological constant
introducedBy Albert Einstein
invariantUnder general coordinate transformations
numberOfIndependentEquations 10
order second-order partial differential equations
predicts black holes
gravitational lensing
gravitational time dilation
gravitational waves
publishedIn Annalen der Physik
reducesTo Newtonian gravity in the weak-field limit
relates geometry of spacetime to matter and energy
spacetimeDimensionAssumed 4
symbolicallyWrittenAs G_{\mu\nu} + \Lambda g_{\mu\nu} = \frac{8\pi G}{c^4} T_{\mu\nu}
tensorRank 2
type nonlinear equations
usedIn astrophysics
cosmological models
gravitational wave modeling
numerical relativity
uses Einstein tensor
Ricci curvature tensor
Ricci scalar
metric tensor
stress–energy tensor
yearProposed 1915

Referenced by (24)

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

Ricci curvature tensor appearsIn Einstein field equations
Ricci scalar appearsIn Einstein field equations
Einstein tensor appearsInEquation Einstein field equations
Newtonian gravitational constant G appearsInEquation Einstein field equations
this entity surface form: Einstein field equations (via κ = 8πG/c^4)
black hole no-hair theorem assumes Einstein field equations
Einstein–Maxwell equations basedOn Einstein field equations
Oppenheimer–Volkoff limit basedOn Einstein field equations
Schwarzschild Penrose diagram basedOn Einstein field equations
Einstein–Rosen bridge basedOnSolutionOf Einstein field equations
On the Curvature of Space basedOnTheory Einstein field equations
theory of relativity coreConcept Einstein field equations
general relativity coreEquation Einstein field equations
FLRW cosmological models governedBy Einstein field equations
this entity surface form: Friedmann equations
Arthur Geoffrey Walker hasResearchInterest Einstein field equations
Albert Einstein knownFor Einstein field equations
The Mathematical Theory of Black Holes mainSubject Einstein field equations
Lorentzian geometry providesFrameworkFor Einstein field equations
Einstein–Maxwell equations relatedTo Einstein field equations
this entity surface form: Einstein equations
On the Curvature of Space relatedTo Einstein field equations
this entity surface form: Friedmann equations
subject surface form: Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie
Christoffel symbols usedIn Einstein field equations
this entity surface form: Einstein field equations formulation
Riemann curvature tensor usedIn Einstein field equations