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.
All labels observed (10)
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 ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
Instruction
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Input
Subject: Einstein field equations Description of subject: The Einstein field equations are the core mathematical framework of general relativity, relating the curvature of spacetime to the distribution of matter and energy.
Referenced by (49)
Full triples — surface form annotated when it differs from this entity's canonical label.
this entity surface form:
Friedmann equations
this entity surface form:
Einstein field equations (via κ = 8πG/c^4)
this entity surface form:
Einstein field equations formulation
"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 equations
this entity surface form:
Friedmann equations
this entity surface form:
Einstein field equations with negative cosmological constant
this entity surface form:
Friedmann equations
this entity surface form:
Einstein’s 1915 field equations of general relativity
subject surface form:
A First Course in General Relativity
this entity surface form:
Friedmann equations in cosmology
this entity surface form:
vacuum Einstein equations
this entity surface form:
Einstein field equations with cosmological constant