The General Theory of Relativity was proposed by Albert Einstein in 1915 – ten years after the publication of his Special Theory of Relativity in the journal Annalen der Physik. The general theory incorporates gravity and accelerated frames of reference in the special theory, and may be summarized by the celebrated Einstein’s field equations:
where
and μ, ν ∈ {0,1,2,3} refer to the four spacetime co-ordinates, one (0) for time and three (1, 2, 3) for space. Since μ and ν can each take on four values, there is not one but sixteen field equations. The left-hand side of each equation is an expression involving the curvature of spacetime while the right-hand side deals with energy and momentum. You could say that the equations are trying to tell us the following: “Space tells matter how to move, matter tells space how to curve.”
where
- Rμν is the Ricci curvature tensor,
R is the scalar curvature,
gμν is the metric tensor,
Λ is the cosmological constant,
G is the gravitational constant,
Tμν is the stress–energy–momentum tensor,
and μ, ν ∈ {0,1,2,3} refer to the four spacetime co-ordinates, one (0) for time and three (1, 2, 3) for space. Since μ and ν can each take on four values, there is not one but sixteen field equations. The left-hand side of each equation is an expression involving the curvature of spacetime while the right-hand side deals with energy and momentum. You could say that the equations are trying to tell us the following: “Space tells matter how to move, matter tells space how to curve.”