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Einstein Field Equations


The Einstein field equations are the 16 coupled hyperbolic-elliptic nonlinear partial differential equations that describe the gravitational effects produced by a given mass in general relativity. As result of the symmetry of G_(munu) and T_(munu), the actual number of equations reduces to 10, although there are an additional four differential identities (the Bianchi identities) satisfied by G_(munu), one for each coordinate.

The Einstein field equations state that

 G_(munu)=8piT_(munu),

where T_(munu) is the stress-energy tensor, and

 G_(munu)=R_(munu)-1/2g_(munu)R

is the Einstein tensor, with R_(munu) the Ricci curvature tensor and R the scalar curvature.

The opening sequence of the 2003 French film Les Triplettes de Belleville (The Triplets of Belleville) features the Einstein field equations.


See also

Bianchi Identities, Einstein Tensor, Ricci Curvature Tensor, Scalar Curvature

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Cite this as:

Weisstein, Eric W. "Einstein Field Equations." From MathWorld--A Wolfram Web Resource. https://mathworld.wolfram.com/EinsteinFieldEquations.html

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