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.
Observed surface forms (4)
| Surface form | Occurrences |
|---|---|
| Friedmann equations | 2 |
| Einstein equations | 1 |
| Einstein field equations (via κ = 8πG/c^4) | 1 |
| Einstein field equations formulation | 1 |
Statements (49)
| 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.
this entity surface form:
Einstein field equations (via κ = 8πG/c^4)
this entity surface form:
Friedmann equations
this entity surface form:
Einstein equations
this entity surface form:
Friedmann equations
"Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie"
→
topic
→
Einstein field equations
ⓘ
subject surface form:
Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie
this entity surface form:
Einstein field equations formulation