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In general relativity, the metric tensor (in this context often abbreviated to simply the metric) is the fundamental object of study. The metric captures all the geometric and causal structure of spacetime, being used to define notions such as time, distance, volume, curvature, angle, and separation of the future and the past.
Examples, Local coordinates and matrix representations & Definition
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metric displaystyle tensor mu coordinates nu spacetime relativity local general matrix curvature given schwarzschild equations manifold space components ds interval
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| time | instance of | being used to define notions | 0.80 | text |
| distance | instance of | being used to define notions | 0.80 | text |
| volume | instance of | being used to define notions | 0.80 | text |
| curvature | instance of | being used to define notions | 0.80 | text |
| angle | instance of | being used to define notions | 0.80 | text |
| and separation of the future | instance of | being used to define notions | 0.80 | text |
| the past.In general relativity | instance of | being used to define notions | 0.80 | text |
| the metric tensor plays the role of the gravitational potential in the classical theory of gravitation | instance of | being used to define notions | 0.80 | text |
| although the physical content of the associated equations is entirely different | instance of | being used to define notions | 0.80 | text |
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