In probability theory, Maxwell's theorem (known also as Herschel-Maxwell's theorem and Herschel-Maxwell's derivation) states that if the probability distribution of a random vector in R n {\displaystyle \mathbb {R} ^{n}} is unchanged by rotations, and if the components are independent, then the components are identically distributed and normally distributed.
Equivalent statements If the probability distribution of a vector-valued random variable X = ( X1, ..., Xn )T is the same as the distribution of GX for every n×n orthogonal matrix G and the components are independent, then the components X1, ..., Xn are normally distributed with expected value 0 and all have the same variance. This theorem is one of many characterizations of the normal distribution. The only rotationally invariant probability distributions on Rn that have independent components are multivariate normal distributions with expected value 0 and variance σ2In, (where In = the n×n identity matrix), for some positive number σ2.
History John Herschel proved the theorem in 1850. Ten years later, James Clerk Maxwell proved the theorem in Proposition IV of his 1860 paper.
Proof We only need to prove the theorem for the 2-dimensional case, since we can then generalize the theorem to n-dimensions by sequentially applying the theorem for 2-dimensions to each pair of coordinates. Since rotating by 90 degrees preserves the joint distribution, X 1 {\displaystyle X_{1}} and X 2 {\displaystyle X_{2}} have the same probability measure: let it be μ {\displaystyle \mu } . If μ {\displaystyle \mu } is a Dirac delta distribution at zero, then it is, in particular, a degenerate gaussian distribution. Let us now assume that μ {\displaystyle \mu } is not a Dirac delta distribution at zero. By Lebesgue's decomposition theorem, we can decompose μ {\displaystyle \mu } into a sum of a regular measure and an atomic measure: μ = μ r + μ s {\displaystyle \mu =\mu _{r}+\mu _{s}} . We need to show that μ s = 0 {\displaystyle \mu _{s}=0} ; we proceed by contradiction. Suppose μ s {\displaystyle \mu _{s}} contains an atomic part, then there exists some x ∈ R {\displaystyle x\in \mathbb {R} } such that μ s ( { x } ) > 0 {\displaystyle \mu _{s}(\{x\})>0} . By independence of X 1 , X 2 {\displaystyle X_{1},X_{2}} , the conditional variable X 2 | { X 1 = x } {\displaystyle X_{2}|\{X_{1}=x\}} is distributed the same way as X 2 {\displaystyle X_{2}} . Suppose x = 0 {\displaystyle x=0} , then since we assumed μ {\displaystyle \mu } is not concentrated at zero, P r ( X 2 ≠ 0 ) > 0 {\displaystyle Pr(X_{2}\neq 0)>0} , and so the double ray { ( x 1 , x 2 ) : x 1 = 0 , x 2 ≠ 0 } {\displaystyle \{(x_{1},x_{2}):x_{1}=0,x_{2}\neq 0\}} has nonzero probability. Now, by the rotational symmetry of μ × μ {\displaystyle \mu \times \mu } , any rotation of the double ray also has the same nonzero probability, and since any two rotations are disjoint, their union has infinite probability, which is a contradiction. Let μ {\displaystyle \mu } have probability density function ρ {\displaystyle \rho } ; the problem reduces to solving the functional equation
ρ ( x ) ρ ( y ) = ρ ( x cos θ + y sin θ ) ρ ( x sin θ − y cos θ ) . {\displaystyle \rho (x)\rho (y)=\rho (x\cos \theta +y\sin \theta )\rho (x\sin \theta -y\cos \theta ).}
References
Sources Bryc, Wlodzimierz (1995). The Normal Distribution: Characterizations with Applications. Springer-Verlag. ISBN 978-0-387-97990-8. Feller, William (1966). An Introduction to Probability Theory and its Applications. Vol. II (1st ed.). Wiley. p. 187. Maxwell, James Clerk (1860). "Illustrations of the dynamical theory of gases". Philosophical Magazine. 4th Series. 19: 390–393.
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