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The 19 pages that link to Stress–energy tensor, each with the reason it gives.

• General relativityRelated: It supplies the matter-and-energy content that shapes spacetime curvature.

• Conservation of energyRelated: Its covariant conservation expresses local energy-momentum balance in general relativity.

• Noether's theoremRelated: Spacetime symmetries and diffeomorphism invariance connect Noether identities to its conservation properties.

• Friedmann equationsRelated: Its cosmic-fluid form specifies the matter and radiation sourcing expansion.

• Gravitational redshiftRelated: It determines the spacetime geometry that governs gravitational effects on clocks and light.

• Zero-point energyRelated: In general relativity, this is how vacuum energy would enter gravitational dynamics.

• GravitationRelated: It represents the energy and momentum that source spacetime curvature.

• Bianchi identitiesRelated: The field equations and Bianchi identity imply its covariant conservation when the cosmological constant is fixed.

• Vacuum energyRelated: Its vacuum expectation value determines how vacuum energy gravitates.

• Curved spacetimeRelated: It supplies the matter-and-energy content that sources curvature.

• History of general relativityRelated: It supplies the matter-and-energy side of Einstein’s field equations.

• Positive energy theoremRelated: Energy conditions are stated as restrictions on this tensor.

• Mathematics of general relativityRelated: It represents the matter and radiation that source spacetime curvature.

• Ricci calculusRelated: Its components form the matter side of Einstein's tensor equations.