MATH 321 – Mathematical Statistics I
October 17, 2026
Definition: A probability space is a triple \((\Omega, \mathcal{F} , P)\), where \(\Omega\) is the sample space, \(\mathcal{F}\) is the event space, and \(P\) is a probability law (or measure).
Definition: A probability law is a function \(P : \mathcal{F} \to [0,\, 1]\) that maps an event \(A\) to a real number in \([0,\, 1]\). The function must satisfy the axioms of probability:
Non-Negativity: \(P(A) \ge 0\), for any \(A \in \mathcal{F}\).
Normalization: \(P(\Omega) = 1\).
Additivity: For any pairwise disjoint events \(\{A_1,\, A_2,\, A_3,\, \dots \}\), it must be true that \[ P \left( \bigcup_{i=1}^\infty A_i \right) = \sum_{i=1}^\infty P(A_i). \]
We have two models for a probability law:
Theorem: A PMF should satisfy the condition that: \[ \sum_{x \in X(\Omega)} p_X(x) = 1 \]
Let’s now generalize this to continuous random variables.
A probability density function \(f_X\) of a random variable \(X\) is a mapping \(f_X : X(\Omega) \to \mathbb{R}\), with the properties
We take \(f_X(x) = 0\) for any \(x \notin X(\Omega)\).
Any function \(f(x)\) satisfying these properties defines a probability law using integration.
Let \(X\) be a continuous random variable. The probability density function of \(X\) is a function \(f_X : X(\Omega) \to \mathbb{R}\) that, when integrated over an interval \([a,\, b]\), yields the probability of obtaining \(a \le X \le b\): \[ P[a \le X \le b] = \int_a^b f_X(x) \, dx. \]
The probability density function uniquely determines the distribution of a random variable. If \(X(\Omega) = Y(\Omega)\) and \(f_X(t) = f_Y(t)\) for all \(t \in X(\Omega)\), then \(X\) and \(Y\) have the same distribution (but need not be equal as random variables).
Example: Let \(f_X(x) = 3x^2\) with \(X(\Omega) = [0, 1]\).
Let \(X\) be a continuous random variable. The cumulative distribution function (CDF) of \(X\) is: \[ F_X(x) \overset{def}{=} P[X \le x] = \int_{-\infty}^x f_X(t) \, dt. \]
Let \(X\) be a continuous random variable. Then, for any \(a \le b\): \[ P[a \le X \le b] = F_X(b) - F_X(a) \]
The survival function of \(X\) is: \[ S_X(x) = 1 - F_X(x) \overset{def}{=} P[X > x] = \int_{x}^\infty f_X(t) \, dt. \]
The probability density function (PDF) is the derivative of the cumulative distribution function (CDF): \[ f_X(x) = \frac{d}{dx} F_X(x), \] provided \(F_X\) is differentiable at \(x\).
If \(F_X\) has a jump discontinuity at \(x = x_0\), then \(f_X(x)\) contains the term \[ P[X = x_0] \, \delta(x - x_0). \]
Example: Let \(f_X(x) = 3x^2\) with \(X(\Omega) = [0, 1]\).
Theorem: Let \(X\) be a random variable (either continuous or discrete), then the CDF of \(X\) has the following properties:
Theorem: For any random variable \(X\) (discrete or continuous), \(F_X(x)\) is always right-continuous. That is, \[ F_X(b) = F_X(b^+) \overset{def}{=} \lim_{h \to 0^+} F_X(b + h). \]
Theorem: For any random variable \(X\) (discrete or continuous), \(P(X = b)\) is: \[ P[X = b] = \begin{cases} F_X(b) - F_X(b^-), & \text{if $F_X$ is discontinuous at $x = b$,} \\ 0, & \text{otherwise}, \end{cases} \] where \(F_X(b^-) \overset{def}{=} \displaystyle\lim_{h \to 0^+} F_X(b - h)\).
We can generalize the definition of the expected value we developed with discrete random variables and sums to continuous random variables and integrals.
The expectation of a continuous random variable \(X\) is: \[ E[X] = \int_{X(\Omega)} x f_X(x) \, dx. \]
Theorem: Let \(g : X(\Omega) \to \mathbb{R}\) be a function and \(X\) be a continuous random variable. Then: \[ E\Big[ g(X) \Big] = \int_{X(\Omega)} g(x) f_X(x) \, dx. \]
The \(n^{th}\) moment of a continuous random variable \(X\) is \[ E[X^n] = \int_{X(\Omega)} x^n f_X(x) \, dx. \]
The \(n^{th}\) central moment of a continuous random variable \(X\) is \[ E[(X-\mu)^n] = \int_{X(\Omega)} (x-\mu)^n f_X(x) \, dx, \] where \(\mu = E[X]\).
The same thing applies to the variance.
The variance of a continuous random variable \(X\) is: \[ V[X] = \int_{X(\Omega)} (x-\mu)^2 f_X(x) \, dx. \]
The formulas concerning the variance and the expected value hold, such as \(V(X) = E(X^2) - [E(X)]^2\).
Example: Let \(f_X(x) = 3x^2\) with \(X(\Omega) = [0, 1]\).
Let \(X\) be a continuous uniform random variable.
The probability density function of \(X\) is: \[ f_X(x) = \begin{cases} \dfrac{1}{b-a}, & a \le x \le b, \\ 0, & \text{otherwise}, \end{cases} \] where \([a, b]\) is the interval on which \(X\) is defined.
We write \[ X \sim \text{Uniform}(a, b) \] to mean that \(X\) is drawn from a uniform distribution on an interval \([a, b]\).
The mean of a uniformly distributed random variable is: \[ E(X) = \frac{a + b}{2}. \]
Note that this is the midpoint of the interval on which \(X\) is defined.
The variance of a uniformly distributed random variable is: \[ V(X) = \frac{(b-a)^2}{12}. \]
Example: Suppose a train has a uniform probability of arriving between 0 and 10 minutes late.
Let \(X\) be an exponential random variable.
The probability density function of \(X\) is: \[ f_X(x) = \begin{cases} \dfrac{1}{\beta} e^{-\frac{x}{\beta}}, & x \ge 0, \\ 0, & \text{otherwise}, \end{cases} \] where \(\beta > 0\) is a parameter.
We write \[ X \sim \text{Exponential}(\beta) \] to mean that \(X\) is drawn from an exponential distribution of parameter \(\beta\).
The mean of an exponentially distributed random variable is: \[ E(X) = \beta. \]
The variance of an exponentially distributed random variable is: \[ V(X) = \beta^2. \]
Example: Suppose a train is always late but the distribution of (late) arrival times is given by an exponential distribution with \(\beta = 5\).
Let \(X\) be a gamma random variable.
The probability density function of \(X\) is: \[ f_X(x) = \begin{cases} \dfrac{1}{\Gamma(\alpha) \beta^\alpha} x^{\alpha - 1} e^{-\frac{x}{\beta}}, & x \ge 0, \\ 0, & \text{otherwise}, \end{cases} \] where \(\alpha > 0\) (shape) and \(\beta > 0\) (scale) are two parameters.
\(\Gamma(z)\) is the gamma function, defined for \(z > 0\) as: \[ \Gamma(z) = \int_0^\infty t^{z - 1} e^{-t} \, dt. \]
More usefully, for \(z > 1\), this function has the property: \[ \Gamma(z) = (z - 1) \Gamma(z - 1). \]
If \(z \in \mathbb{Z}^+\), then \(\Gamma(z) = (z-1)!\). Also, \(\Gamma\left( \dfrac{1}{2} \right) = \sqrt{\pi}\).
We write \[ X \sim \text{Gamma}(\alpha, \beta) \] to mean that \(X\) is drawn from a Gamma distribution with parameters \(\alpha\) and \(\beta\).
If \(X \sim \text{Gamma}(\alpha = 1, \beta)\), then \(X \sim \text{Exponential}(\beta)\).
The mean of a Gamma distributed random variable is: \[ E(X) = \alpha \beta. \]
The variance of a Gamma distributed random variable is: \[ V(X) = \alpha \beta^2. \]
Let \(X\) be a beta random variable.
The probability density function of \(X\) is: \[ f_X(x) = \begin{cases} \dfrac{\Gamma(\alpha + \beta)}{\Gamma(\alpha) \Gamma(\beta)} x^{\alpha - 1} (1 - x)^{\beta - 1}, & 0 \le x \le 1, \\ 0, & \text{otherwise}, \end{cases} \] where \(\alpha > 0\) and \(\beta > 0\) are two parameters.
We write \[ X \sim \text{Beta}(\alpha, \beta) \] to mean that \(X\) is drawn from a Beta distribution with parameters \(\alpha\) and \(\beta\).
The mean of a Beta distributed random variable is: \[ E(X) = \frac{\alpha}{\alpha + \beta}. \]
The variance of a Beta distributed random variable is: \[ V(X) = \frac{\alpha \beta}{(\alpha + \beta)^2 (\alpha + \beta + 1)}. \]