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Multivariate Normal Distributions · Tutorial 697 of 994

Characteristic Function of a Gaussian Vector

Learn to derive and interpret the Gaussian vector characteristic function, including the roles of the mean vector and covariance matrix.

Advanced 9 min read

What You'll Learn

  • Define the characteristic function of a random vector.
  • Derive the characteristic function of a scalar normal variable.
  • Obtain the Gaussian vector formula from the linear-combination definition.
  • Interpret the linear and quadratic terms involving the mean and covariance.
  • Calculate the characteristic function for independent and correlated Gaussian vectors.

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.

Definition: For a random vector \(X\) taking values in \(\mathbb{R}^p\), its characteristic function is the map \(\varphi_X:\mathbb{R}^p\to\mathbb{C}\) defined by
$$ \varphi_X(t)=E\!\left[\exp\!\left(i\,t^\mathsf{T}X\right)\right], \qquad t\in\mathbb{R}^p, $$
where \(i^2=-1\), and \(t^\mathsf{T}X=\sum_{j=1}^p t_jX_j\). The expectation exists for every \(t\), since the complex random variable inside it has absolute value \(1\).

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.

Result: If \(Y\sim N(m,v)\), where \(m\in\mathbb{R}\) and \(v\geq 0\), then for every real \(u\),
$$ E[e^{iuY}]=\exp\!\left(ium-\frac{u^2v}{2}\right). $$

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

$$ \psi'(s)=i\int_{-\infty}^{\infty}x e^{isx}g(x)\,dx. $$

Because \(g'(x)=-xg(x)\), integration by parts gives

$$ \int_{-\infty}^{\infty}x e^{isx}g(x)\,dx =-\int_{-\infty}^{\infty} e^{isx}g'(x)\,dx =is\int_{-\infty}^{\infty}e^{isx}g(x)\,dx =is\psi(s). $$

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

$$ E[e^{iuY}] =e^{ium}E[e^{iu\sqrt{v}Z}] =e^{ium}e^{-u^2v/2}. $$

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

$$ E[e^{2iZ}] =\exp\!\left(i(2)(0)-\frac{(2)^2(1)}{2}\right) =e^{-2}. $$

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

Theorem: If \(X\in\mathbb{R}^p\) is Gaussian with mean vector \(\mu\) and covariance matrix \(\Sigma\), then its characteristic function is
$$ \varphi_X(t) =\exp\!\left(i\,t^\mathsf{T}\mu-\frac{1}{2}t^\mathsf{T}\Sigma t\right), \qquad t\in\mathbb{R}^p. $$

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,

$$ \begin{aligned} \varphi_X(t) &=E\!\left[e^{i\,t^\mathsf{T}X}\right]\\ &=E[e^{iY}]\\ &=\exp\!\left(i\,t^\mathsf{T}\mu-\frac{1}{2}t^\mathsf{T}\Sigma t\right). \end{aligned} $$

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

$$ \mu=\begin{pmatrix}1\\-2\end{pmatrix}, \qquad \Sigma=\begin{pmatrix}4&0\\0&9\end{pmatrix}. $$

Evaluate the characteristic function at \(t=(1/2,-1)^\mathsf{T}\). The linear term is

$$ t^\mathsf{T}\mu =\frac12(1)+(-1)(-2) =\frac52. $$

The quadratic term is

$$ t^\mathsf{T}\Sigma t =\frac12(4)\frac12+(-1)(9)(-1) =1+9 =10. $$

Therefore,

$$ \varphi_X(t)=\exp\!\left(\frac52 i-\frac{10}{2}\right) =e^{(5/2)i-5}. $$

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,

$$ |\varphi_X(t)|=\exp\!\left(-\frac12t^\mathsf{T}\Sigma t\right). $$

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

$$ X_1=Z_1,\qquad X_2=1+\frac12Z_1+\frac{\sqrt{3}}{2}Z_2. $$

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

$$ \Sigma=\begin{pmatrix}1&1/2\\1/2&1\end{pmatrix}. $$

For \(t=(2,-1)^\mathsf{T}\), the mean term is \(t^\mathsf{T}\mu=-1\). The covariance quadratic form, including its cross-term, is

$$ t^\mathsf{T}\Sigma t =2^2+(-1)^2+2(2)(-1)\frac12 =4+1-2 =3. $$

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

$$ \mu=\begin{pmatrix}2\\3\end{pmatrix}, \qquad \Sigma=\begin{pmatrix}1&-1\\-1&1\end{pmatrix}. $$

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

$$ t^\mathsf{T}\Sigma t =\sum_{j=1}^p t_j^2\Sigma_{jj} +2\sum_{j<k}t_jt_k\Sigma_{jk}. $$

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.

Key takeaway: For a Gaussian vector, evaluate one scalar projection \(t^\mathsf{T}X\). Its mean supplies \(t^\mathsf{T}\mu\), its variance supplies \(t^\mathsf{T}\Sigma t\), and the scalar normal formula yields \(\varphi_X(t)=\exp(i\,t^\mathsf{T}\mu-\tfrac12t^\mathsf{T}\Sigma t)\).

Check Your Understanding

Use the projection definition and the displayed formula to answer the following.

  1. For \(X\sim N(\mu,\Sigma)\), what are the mean and variance of \(t^\mathsf{T}X\)?
  2. 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?
  3. 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.
  4. In the Gaussian vector characteristic function, which parameter determines the phase, and which determines the magnitude?
  5. Why does deriving the formula through scalar projections also cover a degenerate Gaussian vector?