From a Distribution to Its Characteristic Function
A characteristic function packages a probability distribution into a complex-valued function of a real argument. For the standard distributions in this tutorial, its calculation is direct: sum over the possible values of a discrete random variable, or integrate its density for a continuous one. The resulting formulas are useful only when their parameters and signs are handled correctly, so each calculation below begins with the distribution itself and is checked against a concrete case.
The argument \(t\) is real, but the value of \(\varphi_X(t)\) is generally complex. The factor \(i\) in the exponent is essential. In particular, these calculations use \(e^{itx}\), not \(e^{tx}\), which is the exponential appearing in a moment generating function. No moment assumptions are needed for a characteristic function to exist.
Discrete Distributions: Finite Sums and a Probability Series
Proof. For a Bernoulli random variable, the value is \(0\) with probability \(1-p\) and \(1\) with probability \(p\). The finite-sum definition therefore gives \((1-p)e^{it\cdot0}+pe^{it\cdot1}=1-p+pe^{it}\). This calculation includes \(p=0\) and \(p=1\).
For a binomial random variable, the probability of \(k\) is \(\binom{n}{k}p^k(1-p)^{n-k}\), for \(k=0,\ldots,n\). Substituting those probabilities into the definition and applying the binomial theorem gives $$ \begin{aligned} \varphi(t) &=\sum_{k=0}^{n}\binom{n}{k}p^k(1-p)^{n-k}e^{itk}\\ &=\sum_{k=0}^{n}\binom{n}{k}(pe^{it})^k(1-p)^{n-k}\\ &=(1-p+pe^{it})^n. \end{aligned} $$ The formula also covers \(n=0\), when the variable is identically zero, and \(p=0\) or \(p=1\).
For a Poisson random variable, the probability of \(k\) is \(e^{-\lambda}\lambda^k/k!\), for \(k=0,1,\ldots\). Thus $$ \begin{aligned} \varphi(t) &=\sum_{k=0}^{\infty}e^{-\lambda}\frac{\lambda^k}{k!}e^{itk}\\ &=e^{-\lambda}\sum_{k=0}^{\infty}\frac{(\lambda e^{it})^k}{k!}\\ &=e^{-\lambda}\exp(\lambda e^{it}) =\exp\!\bigl(\lambda(e^{it}-1)\bigr). \end{aligned} $$ The series evaluation uses the exponential power series, which converges for every complex argument. When \(\lambda=0\), the variable is zero with probability one and the displayed formula equals \(1\). In all three cases, setting \(t=0\) gives \(1\), as required by \(\mathbb{E}[e^{i0X}]=1\). \(\square\)
Worked Example: A Bernoulli Variable at \(t=\pi\)
Let \(X\) have a Bernoulli distribution with \(p=\tfrac13\). Its characteristic function is $$ \varphi_X(t)=\frac23+\frac13e^{it}. $$ At \(t=\pi\), \(e^{i\pi}=\cos(\pi)+i\sin(\pi)=-1+0i=-1\), so $$ \varphi_X(\pi)=\frac23+\frac13(-1)=\frac13. $$
Check by the probability sum: the value \(0\) contributes \(\tfrac23e^{i\pi\cdot0}=\tfrac23\), and the value \(1\) contributes \(\tfrac13e^{i\pi\cdot1}=-\tfrac13\). Their sum is \(\tfrac23-\tfrac13=\tfrac13\), matching the formula.
Worked Example: A Binomial Variable at \(t=\tfrac{\pi}{2}\)
Let \(X\) have a binomial distribution with \(n=3\) and \(p=\tfrac12\). Every value \(k=0,1,2,3\) has probability \(\binom{3}{k}/8\), so the characteristic function is $$ \varphi_X(t)=\left(\frac{1+e^{it}}{2}\right)^3. $$ At \(t=\tfrac{\pi}{2}\), \(e^{it}=i\), and hence $$ \varphi_X\!\left(\frac{\pi}{2}\right) =\left(\frac{1+i}{2}\right)^3 =\frac{(1+i)^3}{8} =\frac{-2+2i}{8} =\frac{-1+i}{4}. $$
Check by the finite sum: multiplying the sum by \(8\), its four terms are \(1\), \(3i\), \(3e^{i\pi}=-3\), and \(e^{i3\pi/2}=-i\). The sum is therefore \((1+3i-3-i)/8=(-2+2i)/8=(-1+i)/4\), as obtained from the formula.
Worked Example: A Poisson Variable at \(t=\pi\)
Let \(X\) have a Poisson distribution with \(\lambda=2\). At \(t=\pi\), \(e^{i\pi}=-1\), and the formula gives $$ \varphi_X(\pi)=\exp\!\bigl(2(-1-1)\bigr)=e^{-4}. $$
Check by the probability series: substituting \(e^{i\pi k}=(-1)^k\) into the defining sum gives $$ \varphi_X(\pi)=e^{-2}\sum_{k=0}^{\infty}\frac{(-2)^k}{k!} =e^{-2}e^{-2}=e^{-4}. $$ The second equality is the exponential power series evaluated at \(-2\), confirming the result directly.
Continuous Distributions: Density Integrals
Proof. For the exponential density, the definition gives $$ \varphi_X(t)=\int_0^\infty e^{itx}\lambda e^{-\lambda x}\,dx =\lambda\int_0^\infty e^{-(\lambda-it)x}\,dx. $$ Since \(\lambda>0\), the real part of \(\lambda-it\) is positive, and \(e^{-(\lambda-it)x}\) tends to zero as \(x\) tends to infinity. Evaluating the antiderivative, $$ \lambda\left[\frac{-e^{-(\lambda-it)x}}{\lambda-it}\right]_{0}^{\infty} =\frac{\lambda}{\lambda-it}. $$ This establishes the exponential formula, including its convergence condition.
For the normal formula, first take a standard normal random variable \(Z\), whose density is \(g(x)=(2\pi)^{-1/2}e^{-x^2/2}\), and write $$ I(t)=\int_{-\infty}^{\infty}e^{itx}g(x)\,dx. $$ Differentiation under the integral is valid because the absolute value of the derivative of the integrand is \(|x|g(x)\), which is integrable. It follows that \(I'(t)=i\int_{-\infty}^{\infty}xe^{itx}g(x)\,dx\). Since \(g'(x)=-xg(x)\), this becomes \(I'(t)=-i\int_{-\infty}^{\infty}e^{itx}g'(x)\,dx\). Integration by parts has zero boundary term because \(g(x)\) tends to zero at both ends and \(|e^{itx}|=1\). Therefore $$ \int_{-\infty}^{\infty}e^{itx}g'(x)\,dx =-it\int_{-\infty}^{\infty}e^{itx}g(x)\,dx=-itI(t), $$ so \(I'(t)=-tI(t)\). Also \(I(0)=1\), since \(g\) is a probability density. Multiplying the differential equation by \(e^{t^2/2}\) gives \(\frac{d}{dt}(e^{t^2/2}I(t))=0\); its constant value is \(1\) at \(t=0\). Hence \(I(t)=e^{-t^2/2}\).
For a normal random variable \(X\) with mean \(\mu\) and variance \(\sigma^2>0\), substitute \(x=\mu+\sigma z\) in its density integral. The density times \(dx\) becomes \(g(z)\,dz\), and the exponential factor becomes \(e^{it(\mu+\sigma z)}\). Thus $$ \varphi_X(t)=e^{i\mu t}\int_{-\infty}^{\infty}e^{i(\sigma t)z}g(z)\,dz =e^{i\mu t}I(\sigma t) =\exp\!\left(i\mu t-\frac{\sigma^2t^2}{2}\right). $$ This proves both continuous-distribution formulas. \(\square\)
Worked Example: An Exponential Variable at \(t=1\)
Let \(X\) have an exponential distribution with rate \(\lambda=2\). Its characteristic function at \(t=1\) is $$ \varphi_X(1)=\frac{2}{2-i} =\frac{2(2+i)}{(2-i)(2+i)} =\frac{4+2i}{5}. $$
Check from the density integral: the integral is \(2\int_0^\infty e^{-(2-i)x}\,dx\). Its antiderivative gives \(2/(2-i)\), because the exponential term tends to zero at infinity when its exponent has real part \(-2x\). Rationalizing the denominator gives \((4+2i)/5\), the same value. At \(t=0\), the general formula gives \(2/2=1\), also confirming normalization.
Worked Example: A Normal Variable at \(t=1\)
Let \(X\) have a normal distribution with mean \(\mu=1\) and variance \(\sigma^2=4\), so \(\sigma=2\). The formula gives $$ \varphi_X(1)=\exp\!\left(i\cdot1-\frac{4\cdot1^2}{2}\right)=e^{-2+i}=e^{-2}(\cos 1+i\sin 1). $$
Check by standardizing in the integral: substituting \(x=1+2z\) in the normal density integral gives the factor \(e^{i(1+2z)}=e^i e^{i2z}\) and leaves the standard normal density in \(z\). The remaining integral is \(I(2)=e^{-2^2/2}=e^{-2}\), so the result is \(e^i e^{-2}\), exactly the value above. At \(t=0\), the formula gives \(e^0=1\).
Reading and Checking the Formulas
The finite-sum and integral calculations share one check: at \(t=0\), every characteristic function must equal \(1\). This follows directly from its definition, but it is also a useful way to detect missing probability mass or a misplaced parameter. For instance, the exponential expression \(\lambda/(\lambda-it)\) gives \(1\) at zero only when its numerator and rate in the denominator agree.
A second useful check is to keep the complex argument intact until the calculation is finished. For the exponential density, the integral involves \(\lambda-it\), not \(\lambda-t\). For the normal density, the location contributes \(i\mu t\), while the variance contributes the real, nonpositive term \(-\sigma^2t^2/2\). These signs are consistent with the fact that a characteristic function has absolute value at most \(1\): for the normal formula its absolute value is \(e^{-\sigma^2t^2/2}\le1\), and for the exponential formula it is \(\lambda/\sqrt{\lambda^2+t^2}\le1\).
Common mistake: substituting a real argument into an MGF formula. For an exponential variable with rate \(2\), an incorrect calculation might take the MGF expression \(2/(2-s)\) and put \(s=1\), obtaining \(2\). That cannot be the characteristic function at \(t=1\), since its absolute value would exceed \(1\). The correct substitution is \(s=it\), yielding \(2/(2-i)=(4+2i)/5\), whose absolute value is \(2/\sqrt{5}\le1\). The same distinction matters for a normal variable: the location term is \(i\mu t\), not \(\mu t\).
Check Your Understanding
Use the defining sum or integral as well as the relevant formula to check your answers.
- For a Bernoulli random variable with \(p=\tfrac14\), calculate \(\varphi_X(\pi)\) directly from its two possible values.
- For a binomial random variable with \(n=2\) and \(p=\tfrac13\), write the three-term finite sum for \(\varphi_X(t)\), then simplify it to the power formula.
- Evaluate the characteristic function of a Poisson random variable with parameter \(\lambda=1\) at \(t=0\), using its probability series.
- For an exponential random variable with rate \(\lambda=3\), calculate \(\varphi_X(2)\) and rationalize its denominator.
- For a normal random variable with mean \(\mu=0\) and variance \(\sigma^2=1\), evaluate \(\varphi_X(t)\) and state its value at \(t=0\).