[proofplan] We identify the ordinary Gaussian likelihood ratio as $\Lambda_n^{n/2}$, where $\Lambda_n$ is Wilks' determinant lambda computed from the formally defined sample covariance blocks. The unrestricted covariance model has $pq$ more free parameters than the null model, so Wilks' likelihood-ratio theorem gives the limiting $\chi^2_{pq}$ law for $-n\log\Lambda_n$ on the probability-one eventual domain where the sample covariance determinants are nonzero. Multiplying first by $(n-1)/n$ and then by the Bartlett factor $\bigl(n-1-(p+q+1)/2\bigr)/(n-1)$ changes the statistic only by deterministic factors tending to $1$, so Slutsky's theorem preserves the same first-order limiting distribution. [/proofplan] [step:Identify Wilks' lambda as the Gaussian likelihood-ratio statistic] For $x_1,\dots,x_n \in \mathbb{R}^{p+q}$, define the sample mean $\bar x_n\in\mathbb{R}^{p+q}$ and the unbiased sample covariance matrix $S_n\in\mathbb{R}^{(p+q)\times(p+q)}$ by \begin{align*} \bar x_n &:= \frac{1}{n}\sum_{i=1}^n x_i, \\ S_n &:= \frac{1}{n-1}\sum_{i=1}^n (x_i-\bar x_n)(x_i-\bar x_n)^\top. \end{align*} Write the block decomposition of $S_n$ according to the split $\mathbb{R}^{p+q}=\mathbb{R}^p\times\mathbb{R}^q$ as \begin{align*} S_n= \begin{pmatrix} S_{11,n} & S_{12,n} \\ S_{21,n} & S_{22,n} \end{pmatrix}, \end{align*} where $S_{11,n}\in\mathbb{R}^{p\times p}$ and $S_{22,n}\in\mathbb{R}^{q\times q}$ are the diagonal sample covariance blocks. Define the Gaussian log-likelihood function \begin{align*} \ell_n:\mathbb{R}^{p+q}\times \mathcal{S}_{++}^{p+q} &\to \mathbb{R} \\ (m,A) &\mapsto -\frac{n(p+q)}{2}\log(2\pi) -\frac{n}{2}\log\det A -\frac{1}{2}\sum_{i=1}^n (x_i-m)^\top A^{-1}(x_i-m), \end{align*} where $\mathcal{S}_{++}^{p+q}$ denotes the set of positive definite symmetric $(p+q)\times(p+q)$ real matrices. With this notation, the unrestricted maximum likelihood estimator of the mean is $\bar x_n$, and the unrestricted maximum likelihood estimator of the covariance matrix is \begin{align*} \widehat\Sigma_n := \frac{1}{n}\sum_{i=1}^n (x_i-\bar x_n)(x_i-\bar x_n)^\top = \frac{n-1}{n}S_n. \end{align*} Under the null model $\Sigma_{12}=0$, the covariance matrix is block diagonal, and the restricted covariance maximum likelihood estimator is \begin{align*} \widehat\Sigma_{0,n} := \begin{pmatrix} \frac{n-1}{n}S_{11,n} & 0 \\ 0 & \frac{n-1}{n}S_{22,n} \end{pmatrix}. \end{align*} Substituting these maximizers into the likelihood gives the likelihood-ratio statistic \begin{align*} \Lambda_n &= \frac{\sup\{\exp(\ell_n(m,A)):\ A_{12}=0\}} {\sup\{\exp(\ell_n(m,A)):\ A\in \mathcal{S}_{++}^{p+q}\}} \\ &= \frac{\det \widehat\Sigma_n}{\det \widehat\Sigma_{0,n}} = \frac{\det S_n}{\det S_{11,n}\det S_{22,n}}. \end{align*} Thus the statistic in the statement is Bartlett's corrected form of Wilks' likelihood-ratio statistic for the Gaussian independence hypothesis. [/step] [step:Compute the number of restrictions imposed by the null model] The unrestricted covariance parameter space $\mathcal{S}_{++}^{p+q}$ is an open subset of the real [vector space](/page/Vector%20Space) of symmetric $(p+q)\times(p+q)$ matrices, so its dimension is \begin{align*} \frac{(p+q)(p+q+1)}{2}. \end{align*} Under $H_0$, the covariance matrix is block diagonal with one positive definite $p\times p$ block and one positive definite $q\times q$ block. Hence the null covariance parameter space has dimension \begin{align*} \frac{p(p+1)}{2}+\frac{q(q+1)}{2}. \end{align*} The difference between these dimensions is \begin{align*} \frac{(p+q)(p+q+1)}{2} - \frac{p(p+1)}{2} - \frac{q(q+1)}{2} = pq. \end{align*} Therefore the null hypothesis imposes exactly $pq$ independent smooth restrictions on the unrestricted covariance model, namely the vanishing of the $pq$ entries of $\Sigma_{12}$. [/step] [step:Apply Wilks' theorem to obtain the uncorrected chi-squared limit] Let the full parameter space be \begin{align*} \Theta := \mathbb{R}^{p+q}\times \mathcal{S}_{++}^{p+q}, \end{align*} and let the null parameter space be \begin{align*} \Theta_0 := \{(m,A)\in \Theta : A_{12}=0\}. \end{align*} The mean parameter $m\in\mathbb{R}^{p+q}$ is unrestricted in both models, so it is a nuisance parameter common to the full and null parameter spaces. The multivariate normal model is a regular finite-dimensional parametric model: the true parameter $(m_0,A_0)$ lies in the interior of $\Theta$ because $A_0\in\mathcal{S}_{++}^{p+q}$, it lies in the relative interior of $\Theta_0$ under $H_0$ whenever $A_{0,11}$ and $A_{0,22}$ are positive definite, the log-likelihood is twice continuously differentiable in a neighbourhood of $(m_0,A_0)$, and the Fisher information for the Gaussian mean-covariance parameter is nonsingular. The null model is a smooth embedded submodel of codimension $pq$, as computed above. Let $E_n$ be the event that $S_n$, $S_{11,n}$, and $S_{22,n}$ are positive definite. Under the nonsingular multivariate normal law, the centered observations span $\mathbb{R}^{p+q}$ with probability $1$ whenever $n\ge p+q+1$, and their first $p$ and last $q$ coordinate projections span $\mathbb{R}^p$ and $\mathbb{R}^q$ with probability $1$ whenever $n\ge \max\{p+1,q+1\}$. Hence $\mathbb{P}(E_n)=1$ for all sufficiently large $n$, so the determinant ratio defining $\Lambda_n$ is eventually defined almost surely. Define the ordinary likelihood-ratio statistic \begin{align*} R_n := \frac{\sup\{\exp(\ell_n(m,A)):\ (m,A)\in\Theta_0\}} {\sup\{\exp(\ell_n(m,A)):\ (m,A)\in\Theta\}}. \end{align*} By Wilks' likelihood-ratio theorem (citing a result not yet in the wiki: [Wilks' theorem](/theorems/1431)), applied to the regular model $\Theta$ and the embedded null submodel $\Theta_0$ of codimension $pq$, under $H_0$, \begin{align*} -2\log R_n \xrightarrow{d} \chi^2_{pq}. \end{align*} Using the maximized Gaussian likelihoods computed above, the normalizing constants and residual quadratic terms cancel at the maximizers, giving \begin{align*} R_n &= \left(\frac{\det \widehat\Sigma_n}{\det \widehat\Sigma_{0,n}}\right)^{n/2} = \Lambda_n^{n/2}. \end{align*} Therefore \begin{align*} -2\log R_n = -n\log\Lambda_n, \end{align*} and [Wilks' theorem](/theorems/1864) gives \begin{align*} -n\log\Lambda_n \xrightarrow{d} \chi^2_{pq}. \end{align*} Since $(n-1)/n\to 1$, Slutsky's theorem yields \begin{align*} -(n-1)\log\Lambda_n = \frac{n-1}{n}\bigl(-n\log\Lambda_n\bigr) \xrightarrow{d} \chi^2_{pq}. \end{align*} [/step] [step:Insert Bartlett's correction without changing the limiting law] Define the deterministic correction factor \begin{align*} a_n := \frac{n-1-\frac{p+q+1}{2}}{n-1}. \end{align*} Since $p$ and $q$ are fixed, \begin{align*} \lim_{n\to\infty} a_n = 1. \end{align*} The Bartlett-corrected statistic can be written as \begin{align*} -\left(n-1-\frac{p+q+1}{2}\right)\log\Lambda_n = a_n\bigl(-(n-1)\log\Lambda_n\bigr). \end{align*} Since $a_n \to 1$ and $-(n-1)\log\Lambda_n \xrightarrow{d}\chi^2_{pq}$, Slutsky's theorem gives \begin{align*} -\left(n-1-\frac{p+q+1}{2}\right)\log\Lambda_n \xrightarrow{d} \chi^2_{pq}. \end{align*} This is precisely the asserted first-order large-sample chi-squared approximation with $pq$ degrees of freedom. The argument uses only that the Bartlett factor tends to $1$; it does not assert the stronger second-order Bartlett correction property. [/step]