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Metric tensor (general relativity)

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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Local coordinates and matrix representations

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Volume

Curvature

Einstein's equations

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Metric tensor (general relativity)

Nodes97
Edges96
Triples9
Avg. degree1.98
Density0.020619
Components1

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Important terminology

metric displaystyle tensor mu coordinates nu spacetime relativity local general matrix curvature given schwarzschild equations manifold space components ds interval

Entity relationships Subject–Predicate–Object triples

SubjectPredicateObjectConfidenceSrc
timeinstance ofbeing used to define notions0.80text
distanceinstance ofbeing used to define notions0.80text
volumeinstance ofbeing used to define notions0.80text
curvatureinstance ofbeing used to define notions0.80text
angleinstance ofbeing used to define notions0.80text
and separation of the futureinstance ofbeing used to define notions0.80text
the past.In general relativityinstance ofbeing used to define notions0.80text
the metric tensor plays the role of the gravitational potential in the classical theory of gravitationinstance ofbeing used to define notions0.80text
although the physical content of the associated equations is entirely differentinstance ofbeing used to define notions0.80text

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