general relativity
E46425
General relativity is Albert Einstein’s theory of gravitation that describes gravity as the curvature of spacetime caused by mass and energy, successfully explaining phenomena from planetary orbits to black holes and gravitational waves.
Aliases (2)
Statements (50)
| Predicate | Object |
|---|---|
| instanceOf |
geometric theory of gravity
→
physical theory → relativistic field theory → theory of gravitation → |
| appliesTo |
high velocities
→
strong gravitational fields → |
| assumes |
constancy of speed of light locally
→
local Lorentz invariance → |
| basedOn |
equivalence principle
→
principle of general covariance → |
| coreEquation |
Einstein field equations
→
|
| describes |
gravitation
→
gravity as curvature of spacetime → |
| domain |
astrophysics
→
cosmology → macroscopic scales → |
| field |
gravitational physics
→
theoretical physics → |
| formulatedBy |
Albert Einstein
→
|
| generalizes |
special relativity
→
|
| historicalPrecursor |
Einstein’s 1907 equivalence principle paper
→
Einstein’s 1911 gravitational redshift work → |
| includes |
Friedmann–Lemaître–Robertson–Walker metric
→
Kerr metric → Reissner–Nordström metric → Schwarzschild solution → |
| incompatibleWith |
standard formulation of quantum mechanics
→
|
| mathematicalFramework |
Riemannian geometry
→
differential geometry → |
| motivates |
search for quantum gravity
→
|
| predicts |
bending of light by gravity
→
black holes → cosmological expansion solutions → frame dragging → gravitational redshift → gravitational time dilation → gravitational waves → perihelion precession of Mercury → |
| publicationYear |
1915
→
|
| relates |
spacetime curvature to energy-momentum
→
|
| replaces |
Newtonian theory of gravitation
→
|
| testedBy |
Eddington 1919 solar eclipse expedition
→
GPS time dilation corrections → Gravity Probe B experiment → LIGO gravitational wave detections → binary pulsar observations → |
| usesConcept |
curvature tensor
→
geodesics → metric tensor → spacetime manifold → |