From Coordinate Covariations to a Matrix
For a one-dimensional Brownian motion, the quadratic variation over \([0,t]\) is \(t\). In several dimensions, each coordinate has its own quadratic variation, but different coordinates may also accumulate nonzero covariation. Collecting these quantities into a matrix makes it possible to compute the covariations of any linear combinations by ordinary matrix multiplication.
Work on a filtered probability space \((\Omega,\mathcal{F},(\mathcal{F}_t)_{t\ge0},\mathbb{P})\). A \(d\)-dimensional Brownian motion with covariance matrix \(\Gamma\) is an adapted, continuous process \(\mathbf{B}_t=(B_t^1,\ldots,B_t^d)^{\mathsf T}\), with \(\mathbf{B}_0=0\), whose increments after time \(s\) are independent of \(\mathcal{F}_s\) and whose increment \(\mathbf{B}_t-\mathbf{B}_s\) is a centered Gaussian vector with covariance \((t-s)\Gamma\), for \(0\le s<t\). Here \(\Gamma\) is a fixed symmetric positive semidefinite \(d\times d\) matrix. Its entries satisfy \(\mathbb{E}[(B_t^i-B_s^i)(B_t^j-B_s^j)]=(t-s)\Gamma_{ij}\).
When \(\Gamma=I_d\), the coordinates are independent standard Brownian motions. If \(\Gamma_{ii}=1\) for every \(i\), the coordinates each have standard Brownian variance, but they need not be independent. For positive diagonal entries, their instantaneous correlation is \(\Gamma_{ij}/\sqrt{\Gamma_{ii}\Gamma_{jj}}\). A singular \(\Gamma\) is allowed: it means that some nonzero linear combination of the coordinates has zero variance.
The Covariation Matrix Theorem
Proof. Fix \(T>0\) and a deterministic partition \(0=t_0<\cdots<t_n=T\). Write \(\Delta t_k=t_k-t_{k-1}\), \(\Delta B_k^i=B_{t_k}^i-B_{t_{k-1}}^i\), and \(S_\Pi^{ij}=\sum_k\Delta B_k^i\Delta B_k^j\). The Gaussian increment covariance gives \(\mathbb{E}[\Delta B_k^i\Delta B_k^j]=\Gamma_{ij}\Delta t_k\), so \(\mathbb{E}[S_\Pi^{ij}]=T\Gamma_{ij}\).
For jointly centered Gaussian variables \(X,Y\), with variances \(a,b\) and covariance \(c\), the fourth-moment identity gives \(\mathbb{E}[X^2Y^2]=ab+2c^2\), and hence \(\operatorname{Var}(XY)=ab+c^2\). To verify the identity when \(a>0\), write \(X=\sqrt a\,U\) and \(Y=(c/\sqrt a)U+\sqrt{b-c^2/a}\,V\), where \(U,V\) are independent standard normal variables. Expanding \(X^2Y^2\), using \(\mathbb{E}[U^4]=3\), \(\mathbb{E}[U^2V^2]=1\), and the vanishing of the odd terms gives \(ab+2c^2\). If \(a=0\), then \(X=0\) almost surely and \(c=0\), so the same identity holds.
Apply this identity to each increment pair. Since increments on distinct partition intervals are independent, the products \(\Delta B_k^i\Delta B_k^j\) are independent across \(k\). Their variances therefore add, giving $$ \operatorname{Var}(S_\Pi^{ij}) =\left(\Gamma_{ii}\Gamma_{jj}+\Gamma_{ij}^2\right)\sum_k(\Delta t_k)^2 \le \left(\Gamma_{ii}\Gamma_{jj}+\Gamma_{ij}^2\right)T|\Pi|. $$ Here \(|\Pi|=\max_k\Delta t_k\), and the inequality follows from \(\sum_k(\Delta t_k)^2\le|\Pi|\sum_k\Delta t_k=T|\Pi|\). Thus \(\mathbb{E}[(S_\Pi^{ij}-T\Gamma_{ij})^2]=\operatorname{Var}(S_\Pi^{ij})\to0\) as \(|\Pi|\to0\). Applying the same argument on \([0,t]\) gives the limit \(t\Gamma_{ij}\) for each \(t\). There are only finitely many entries, so the matrix of sums converges entry by entry in \(L^2\) to \(t\Gamma\). The case \(T=0\) has empty sums and the stated limit is zero. \(\square\)
In differential notation, the matrix result is recorded as \(dB_t^i\,dB_t^j=\Gamma_{ij}\,dt\). This is shorthand for the partition-sum limit, not an identity between individual increments. In particular, the diagonal rule is \(dB_t^i\,dB_t^i=\Gamma_{ii}\,dt\); it equals \(dt\) only when that coordinate has unit variance per unit time.
Linear Combinations and Matrix Multiplication
Proof. On any partition, the increment of coordinate \(r\) of \(\mathbf{Y}\) is \(\Delta Y_k^r=\sum_i A_{ri}\Delta B_k^i\). For coordinates \(r,s\), expand the partition sum exactly: $$ \sum_k\Delta Y_k^r\Delta Y_k^s =\sum_i\sum_j A_{ri}A_{sj}\sum_k\Delta B_k^i\Delta B_k^j. $$ Each inner sum converges in \(L^2\) to \(t\Gamma_{ij}\) by the theorem. The sums over \(i,j\) are finite, so the full expression converges to \(t\sum_{i,j}A_{ri}\Gamma_{ij}A_{sj}\), which is the \((r,s)\) entry of \(tA\Gamma A^{\mathsf T}\). Taking \(m=1\) for each of \(a^{\mathsf T}\mathbf{B}\) and \(b^{\mathsf T}\mathbf{B}\), or using the same expansion with two different coefficient vectors, gives the scalar formula. \(\square\)
The transformed matrix is again symmetric positive semidefinite. Indeed, for every \(x\in\mathbb{R}^m\), $$ x^{\mathsf T}A\Gamma A^{\mathsf T}x=(A^{\mathsf T}x)^{\mathsf T}\Gamma(A^{\mathsf T}x)\ge0, $$ because \(\Gamma\) is positive semidefinite. Thus the variance rate of every scalar combination \(a^{\mathsf T}\mathbf{B}\) is \(a^{\mathsf T}\Gamma a\), which cannot be negative.
Worked Example: Sum and Difference of Correlated Coordinates
Suppose \(\Gamma=\begin{pmatrix}1&3/5\\3/5&1\end{pmatrix}\), and set \(Y_t=B_t^1+B_t^2\) and \(Z_t=B_t^1-B_t^2\). Find their quadratic variations and covariation.
The coefficient matrix is \(A=\begin{pmatrix}1&1\\1&-1\end{pmatrix}\). First multiply: $$ A\Gamma =\begin{pmatrix}1&1\\1&-1\end{pmatrix} \begin{pmatrix}1&3/5\\3/5&1\end{pmatrix} =\begin{pmatrix}8/5&8/5\\2/5&-2/5\end{pmatrix}. $$ Then $$ A\Gamma A^{\mathsf T} =\begin{pmatrix}8/5&8/5\\2/5&-2/5\end{pmatrix} \begin{pmatrix}1&1\\1&-1\end{pmatrix} =\begin{pmatrix}16/5&0\\0&4/5\end{pmatrix}. $$ Consequently, \([Y]_t=16t/5\), \([Z]_t=4t/5\), and \([Y,Z]_t=0\).
Check: Direct expansion gives \([Y]_t=(1+1+2(3/5))t=16t/5\) and \([Z]_t=(1+1-2(3/5))t=4t/5\). The cross terms in \([Y,Z]\) cancel: \((1-3/5+3/5-1)t=0\). The original matrix is valid because its leading principal minors are \(1\) and \(1-9/25=16/25>0\).
Worked Example: Transforming Three Correlated Coordinates
Let the covariance matrix and transformation be $$ \Gamma=\begin{pmatrix}1&1/2&0\\1/2&1&1/2\\0&1/2&1\end{pmatrix}, \qquad A=\begin{pmatrix}1&1&0\\0&1&-1\end{pmatrix}. $$ For \(Y_t=B_t^1+B_t^2\) and \(Z_t=B_t^2-B_t^3\), compute their covariation matrix.
The leading principal minors of \(\Gamma\) are \(1\), \(1-1/4=3/4\), and \(\det(\Gamma)=1/2\), all positive, so this symmetric matrix is positive definite. Multiplication gives $$ A\Gamma =\begin{pmatrix}3/2&3/2&1/2\\1/2&1/2&1/2\end{pmatrix}, \qquad A\Gamma A^{\mathsf T} =\begin{pmatrix}3&1\\1&1\end{pmatrix}. $$ Hence \([Y]_t=3t\), \([Z]_t=t\), and \([Y,Z]_t=t\).
Check: Expanding the first variance gives \([Y]_t=(\Gamma_{11}+\Gamma_{22}+2\Gamma_{12})t=(1+1+1)t=3t\). The second gives \([Z]_t=(\Gamma_{22}+\Gamma_{33}-2\Gamma_{23})t=(1+1-1)t=t\). The cross term is \((\Gamma_{12}-\Gamma_{13}+\Gamma_{22}-\Gamma_{23})t=(1/2-0+1-1/2)t=t\), agreeing with the matrix entry.
Worked Example: A Singular Matrix and a Zero Combination
Let \(U,V\) be independent standard Brownian motions on the same filtered probability space and define \(\mathbf{B}_t=(U_t,V_t,U_t+V_t)^{\mathsf T}\). Find its covariance matrix and verify the covariation of \(B^3-B^1-B^2\).
The coordinate covariations are \([U]_t=t\), \([V]_t=t\), and \([U,V]_t=0\). Since \([U,U+V]_t=t\), \([V,U+V]_t=t\), and \([U+V]_t=2t\), the matrix is $$ [\mathbf{B}]_t=t\Gamma,\qquad \Gamma=\begin{pmatrix}1&0&1\\0&1&1\\1&1&2\end{pmatrix}. $$ Take \(a=(-1,-1,1)^{\mathsf T}\), so \(a^{\mathsf T}\mathbf{B}_t=B_t^3-B_t^1-B_t^2\). Direct multiplication yields \(\Gamma a=(0,0,0)^{\mathsf T}\), and therefore \(a^{\mathsf T}\Gamma a=0\). The proposition gives \([a^{\mathsf T}\mathbf{B}]_t=0\).
Check: By the definition of the coordinates, \(B_t^3-B_t^1-B_t^2=(U_t+V_t)-U_t-V_t=0\) at every time, so its quadratic variation is indeed zero. The matrix is positive semidefinite because \(x^{\mathsf T}\Gamma x=(x_1+x_3)^2+(x_2+x_3)^2\ge0\) for every \(x\in\mathbb{R}^3\), and it is singular because \(\Gamma a=0\).
What the Matrix Records—and a Common Error
The covariance matrix at a fixed time and the quadratic-covariation matrix are related but distinct objects. The increment definition gives \(\operatorname{Cov}(\mathbf{B}_t)=t\Gamma\); the theorem gives \([\mathbf{B}]_t=t\Gamma\) as the limit of products of increments along fine partitions. They have the same deterministic matrix in this Brownian setting, but one is a covariance of a random vector at a fixed time and the other is a process defined through path increments.
The matrix formulation also identifies which combinations have zero covariation. For \(a\in\mathbb{R}^d\), the variance rate of \(a^{\mathsf T}\mathbf{B}\) is \(a^{\mathsf T}\Gamma a\). It is zero exactly when this scalar combination has zero quadratic variation. For a positive semidefinite matrix, \(a^{\mathsf T}\Gamma a=0\) implies \(\Gamma a=0\): diagonalizing \(\Gamma\) shows that every component of \(a\) in a positive-eigenvalue direction must vanish. Thus zero-variance combinations correspond to null directions of \(\Gamma\).
Common mistake: For \(Y=B^1+B^2\), it is incorrect to write \([Y]_t=([B^1]_t+[B^2]_t)\), because this drops the cross terms. The correct expansion is $$ [Y]_t=[B^1]_t+[B^2]_t+2[B^1,B^2]_t =t(\Gamma_{11}+\Gamma_{22}+2\Gamma_{12}). $$ For the first example this gives \(t(1+1+6/5)=16t/5\), not \(2t\). The correction is essential whenever coordinates are correlated, and the matrix product \(A\Gamma A^{\mathsf T}\) includes all such cross terms automatically.
Check Your Understanding
Use the matrix formulas and state any conditions needed for your conclusions.
- If \(\Gamma=\begin{pmatrix}4&1\\1&9\end{pmatrix}\), find the variance rates of \(B^1+B^2\) and \(2B^1-B^2\).
- For a two-dimensional Brownian motion with \(\Gamma_{11}=\Gamma_{22}=1\) and \(\Gamma_{12}=-1/3\), find \([B^1+B^2,B^1-B^2]_t\).
- Explain why \(A\Gamma A^{\mathsf T}\) is positive semidefinite whenever \(\Gamma\) is positive semidefinite.
- Give a reason that a covariance matrix with a nonzero null vector can correspond to coordinates that are linearly dependent.
- Identify the missing term in the incorrect calculation \([B^1+B^2]_t=[B^1]_t+[B^2]_t\), and state the correct formula.