From Gaussian Projections to a Vector Transform
A multivariate Gaussian vector can be studied through its one-dimensional projections: for each fixed vector \(t\), the quantity \(t^\mathsf{T}X\) is normal. This fact gives a direct route to the vector’s characteristic function. Rather than integrating a multivariate density—which may not even exist in a singular case—we evaluate one scalar normal characteristic function at a time.
The result is compact, but its two terms have distinct roles. The mean vector contributes a linear expression in \(t\), while the covariance matrix contributes a quadratic expression. Deriving the formula makes clear why every covariance, including an off-diagonal covariance, matters.
Use the linear-combination definition of multivariate normality: \(X\) is Gaussian if every scalar projection \(a^\mathsf{T}X\), for \(a\in\mathbb{R}^p\), has a univariate normal distribution, with a constant allowed as a degenerate normal variable. In the parameterization used here, the projection in direction \(a\) has mean \(a^\mathsf{T}\mu\) and variance \(a^\mathsf{T}\Sigma a\), where \(\mu\in\mathbb{R}^p\) and \(\Sigma\) is the covariance matrix. The latter quantity is nonnegative for every \(a\).
The Scalar Normal Characteristic Function
The vector calculation depends on the characteristic function of a univariate normal variable. We derive it first, including the case of zero variance. This also makes explicit the analytic step used in the calculation.
Proof. First let \(Z\sim N(0,1)\), with density \(g(x)=(2\pi)^{-1/2}e^{-x^2/2}\), and write \(\psi(s)=E[e^{isZ}]\). Since \(|x|g(x)\) is integrable, differentiation under the integral is justified by dominated convergence: the absolute value of the derivative of \(e^{isx}g(x)\) with respect to \(s\) is \(|x|g(x)\), independently of \(s\). Thus
Because \(g'(x)=-xg(x)\), integration by parts gives
The boundary term vanishes because \(g(x)\to0\) as \(x\to\pm\infty\), while \(|e^{isx}|=1\). It follows that \(\psi'(s)=-s\psi(s)\), with \(\psi(0)=1\). Solving this differential equation gives \(\psi(s)=e^{-s^2/2}\). If \(v>0\), write \(Y=m+\sqrt{v}\,Z\); then
If \(v=0\), \(Y=m\) with probability one, so \(E[e^{iuY}]=e^{ium}\), which is the same formula with \(v=0\). \(\square\)
Worked Example: A Standard Normal Variable
Let \(Z\sim N(0,1)\). At frequency \(u=2\), the scalar formula gives
The value is real and positive because the mean is zero; there is no linear phase term. The exponent’s real part is \(-2\), from the variance contribution.
Deriving the Gaussian Vector Formula
Proof. Fix an arbitrary \(t\in\mathbb{R}^p\). By the linear-combination definition, \(Y=t^\mathsf{T}X\) is a scalar normal variable. Its mean is \(t^\mathsf{T}\mu\) and its variance is \(t^\mathsf{T}\Sigma t\). The scalar result applies even if this variance is zero. By the definition of the vector characteristic function,
Since \(t\) was arbitrary, this holds for every \(t\in\mathbb{R}^p\). \(\square\)
The formula also follows directly from the parameters of the projection. In the scalar normal characteristic function, set \(u=1\), \(m=t^\mathsf{T}\mu\), and \(v=t^\mathsf{T}\Sigma t\). The frequency \(t\) is the direction of the projection as well as the argument of the vector characteristic function; it is not a random vector.
Worked Example: Independent Gaussian Components
Suppose \(X_1\sim N(1,4)\) and \(X_2\sim N(-2,9)\) are independent, and let \(X=(X_1,X_2)^\mathsf{T}\). Its mean vector and covariance matrix are
Evaluate the characteristic function at \(t=(1/2,-1)^\mathsf{T}\). The linear term is
The quadratic term is
Therefore,
The same calculation can be checked from the projection: \(t^\mathsf{T}X=X_1/2-X_2\) has mean \(5/2\) and variance \(4(1/2)^2+9=10\), agreeing with the two expressions above.
How the Mean and Covariance Enter
The mean term \(i\,t^\mathsf{T}\mu\) is linear in \(t\). It determines the oscillatory, or phase, part of the characteristic function. The covariance term is real and nonpositive in the exponent, since \(t^\mathsf{T}\Sigma t\geq0\). Consequently,
Thus the covariance controls the magnitude of the characteristic function, while the mean affects its phase. The matrix expression is not merely a sum of marginal variances: it includes the covariances between components.
Worked Example: A Correlated Gaussian Pair
Let \(Z_1,Z_2\) be independent standard normal variables and define
The mean vector is \(\mu=(0,1)^\mathsf{T}\). The variances are \(1\) and \((1/2)^2+(\sqrt{3}/2)^2=1\); the covariance is \(E[Z_1(\frac12Z_1+\frac{\sqrt{3}}2Z_2)]=1/2\). Hence
For \(t=(2,-1)^\mathsf{T}\), the mean term is \(t^\mathsf{T}\mu=-1\). The covariance quadratic form, including its cross-term, is
Therefore \(\varphi_X(t)=\exp(-i-3/2)\). Directly, \(t^\mathsf{T}X=2X_1-X_2=-1+\frac32Z_1-\frac{\sqrt{3}}2Z_2\), which has mean \(-1\) and variance \((3/2)^2+(\sqrt{3}/2)^2=3\). The projection calculation confirms both terms in the formula.
Worked Example: A Degenerate Gaussian Vector
Let \(Z\sim N(0,1)\) and set \(X=(2+Z,\,3-Z)^\mathsf{T}\). This vector lies on a line, but its projections are still normal, including projections that are constant. Its mean and covariance matrix are
At \(t=(1,2)^\mathsf{T}\), \(t^\mathsf{T}\mu=8\) and \(t^\mathsf{T}\Sigma t=(1-2)^2=1\), so \(\varphi_X(t)=e^{8i-1/2}\). Indeed, \(t^\mathsf{T}X=(2+Z)+2(3-Z)=8-Z\), a normal variable with mean \(8\) and variance \(1\). In contrast, \(t=(1,1)^\mathsf{T}\) gives \(t^\mathsf{T}X=5\) with probability one: the quadratic form is zero, and the formula gives \(\varphi_X(t)=e^{5i}\). No density assumption is needed.
Common Pitfall and Why the Formula Matters
A frequent error is to omit the off-diagonal entries of \(\Sigma\) when evaluating \(t^\mathsf{T}\Sigma t\). For a symmetric matrix, expansion gives
The cross-terms can increase or decrease the variance of a projection, depending on the signs of the coefficients and covariances. In the correlated-pair example, dropping the cross-term would give \(5\), not the correct value \(3\).
- Wrong reasoning: “The quadratic term is the sum of squared coefficients times component variances, so covariance entries do not enter.”
- Correction: That sum accounts only for the diagonal terms. The variance of \(t^\mathsf{T}X\) is \(t^\mathsf{T}\Sigma t\), which includes the cross-terms.
- Another check: At \(t=0\), the formula must give \(\varphi_X(0)=1\). At any \(t\), its magnitude must be at most \(1\), as the exponent’s real part is nonpositive.
The projection-based derivation is useful whenever a calculation asks for the characteristic function in a particular direction. It also works for Gaussian vectors whose distributions are concentrated on a lower-dimensional set, because it never requires a multivariate density.
Check Your Understanding
Use the projection definition and the displayed formula to answer the following.
- For \(X\sim N(\mu,\Sigma)\), what are the mean and variance of \(t^\mathsf{T}X\)?
- If \(t^\mathsf{T}\Sigma t=0\), what does the formula say about the magnitude of \(\varphi_X(t)\), and what does that imply about the projection?
- For \(\Sigma=\begin{pmatrix}2&1\\1&3\end{pmatrix}\) and \(t=(1,-1)^\mathsf{T}\), calculate \(t^\mathsf{T}\Sigma t\), showing the cross-term.
- In the Gaussian vector characteristic function, which parameter determines the phase, and which determines the magnitude?
- Why does deriving the formula through scalar projections also cover a degenerate Gaussian vector?