In general relativity, the Raychaudhuri equation, or Landau–Raychaudhuri equation, is a fundamental result describing the motion of nearby bits of matter. The equation is important as a fundamental lemma for the Penrose–Hawking singularity theorems and for the study of exact solutions in general relativity, but has independent interest, since it offers a simple and general validation of our intuitive expectation that gravitation should be a universal attractive force between any two bits of mass–energy in general relativity, as it is in Newton's theory of gravitation. The equation was discovered independently by the Indian physicist Amal Kumar Raychaudhuri and the Soviet physicist Lev Landau.
Mathematical statement Given a timelike unit vector field X → {\displaystyle {\vec {X}}} (which can be interpreted as a family or congruence of nonintersecting world lines via the integral curve, not necessarily geodesics), Raychaudhuri's equation in D {\displaystyle D} spacetime dimensions can be written as
θ ˙ = − θ 2 D − 1 − 2 σ 2 + 2 ω 2 − E [ X → ] a a + X ˙ a ; a {\displaystyle {\dot {\theta }}=-{\frac {\theta ^{2}}{D-1}}-2\sigma ^{2}+2\omega ^{2}-{E[{\vec {X}}]^{a}}_{a}+{{\dot {X}}^{a}}_{;a}}
where
2 σ 2 = σ m n σ m n , 2 ω 2 = ω m n ω m n {\displaystyle 2\sigma ^{2}=\sigma _{mn}\,\sigma ^{mn},\;2\omega ^{2}=\omega _{mn}\,\omega ^{mn}}
are (non-negative) quadratic invariants of the shear tensor
σ a b = θ a b − 1 D − 1 θ h a b {\displaystyle \sigma _{ab}=\theta _{ab}-{\frac {1}{D-1}}\,\theta \,h_{ab}}
and the vorticity tensor
ω a b = h m a h n b X [ m ; n ] {\displaystyle \omega _{ab}={h^{m}}_{a}\,{h^{n}}_{b}X_{[m;n]}}
respectively. Here,
θ a b = h m a h n b X ( m ; n ) {\displaystyle \theta _{ab}={h^{m}}_{a}\,{h^{n}}_{b}X_{(m;n)}}
is the expansion tensor, θ {\displaystyle \theta } is its trace, called the expansion scalar, and
h a b = g a b + X a X b {\displaystyle h_{ab}=g_{ab}+X_{a}\,X_{b}}
is the projection tensor onto the hyperplanes orthogonal to X → {\displaystyle {\vec {X}}} . Also, dot denotes differentiation with respect to proper time counted along the world lines in the congruence. Finally, the trace of the tidal tensor E [ X → ] a b {\displaystyle E[{\vec {X}}]_{ab}} can also be written as
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