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A **random variable** (also called **random quantity**, **aleatory variable**, or **stochastic variable**) is a mathematical formalization of a quantity or object which depends on random events.^{[1]} It is a mapping or a function from possible outcomes (e.g., the possible upper sides of a flipped coin such as heads and tails ) in a sample space (e.g., the set ) to a measurable space, often the real numbers (e.g., in which 1 corresponding to and -1 corresponding to ).

Informally, randomness typically represents some fundamental element of chance, such as in the roll of a dice; it may also represent uncertainty, such as measurement error.^{[1]} However, the interpretation of probability is philosophically complicated, and even in specific cases is not always straightforward. The purely mathematical analysis of random variables is independent of such interpretational difficulties, and can be based upon a rigorous axiomatic setup.

In the formal mathematical language of measure theory, a random variable is defined as a measurable function from a probability measure space (called the *sample space*) to a measurable space. This allows consideration of the pushforward measure, which is called the *distribution* of the random variable; the distribution is thus a probability measure on the set of all possible values of the random variable. It is possible for two random variables to have identical distributions but to differ in significant ways; for instance, they may be independent.

It is common to consider the special cases of discrete random variables and absolutely continuous random variables, corresponding to whether a random variable is valued in a discrete set (such as a finite set) or in an interval of real numbers. There are other important possibilities, especially in the theory of stochastic processes, wherein it is natural to consider random sequences or random functions. Sometimes a *random variable* is taken to be automatically valued in the real numbers, with more general random quantities instead being called *random elements*.

According to George Mackey, Pafnuty Chebyshev was the first person "to think systematically in terms of random variables".^{[2]}

A **random variable** is a measurable function from a sample space as a set of possible outcomes to a measurable space . The technical axiomatic definition requires the sample space to be a sample space of a probability triple (see the measure-theoretic definition). A random variable is often denoted by capital roman letters such as , , , .^{[3]}

The probability that takes on a value in a measurable set is written as

In many cases, is real-valued, i.e. . In some contexts, the term random element (see extensions) is used to denote a random variable not of this form.

When the image (or range) of is countable, the random variable is called a **discrete random variable**^{[4]}^{: 399 } and its distribution is a discrete probability distribution, i.e. can be described by a probability mass function that assigns a probability to each value in the image of . If the image is uncountably infinite (usually an interval) then is called a **continuous random variable**.^{[5]}^{[6]} In the special case that it is absolutely continuous, its distribution can be described by a probability density function, which assigns probabilities to intervals; in particular, each individual point must necessarily have probability zero for an absolutely continuous random variable. Not all continuous random variables are absolutely continuous,^{[7]} a mixture distribution is one such counterexample; such random variables cannot be described by a probability density or a probability mass function.

Any random variable can be described by its cumulative distribution function, which describes the probability that the random variable will be less than or equal to a certain value.

The term "random variable" in statistics is traditionally limited to the real-valued case ( ). In this case, the structure of the real numbers makes it possible to define quantities such as the expected value and variance of a random variable, its cumulative distribution function, and the moments of its distribution.

However, the definition above is valid for any measurable space of values. Thus one can consider random elements of other sets , such as random boolean values, categorical values, complex numbers, vectors, matrices, sequences, trees, sets, shapes, manifolds, and functions. One may then specifically refer to a *random variable of type *, or an * -valued random variable*.

This more general concept of a random element is particularly useful in disciplines such as graph theory, machine learning, natural language processing, and other fields in discrete mathematics and computer science, where one is often interested in modeling the random variation of non-numerical data structures. In some cases, it is nonetheless convenient to represent each element of , using one or more real numbers. In this case, a random element may optionally be represented as a vector of real-valued random variables (all defined on the same underlying probability space , which allows the different random variables to covary). For example:

- A random word may be represented as a random integer that serves as an index into the vocabulary of possible words. Alternatively, it can be represented as a random indicator vector, whose length equals the size of the vocabulary, where the only values of positive probability are , , and the position of the 1 indicates the word.
- A random sentence of given length may be represented as a vector of random words.
- A random graph on given vertices may be represented as a matrix of random variables, whose values specify the adjacency matrix of the random graph.
- A random function may be represented as a collection of random variables , giving the function's values at the various points in the function's domain. The are ordinary real-valued random variables provided that the function is real-valued. For example, a stochastic process is a random function of time, a random vector is a random function of some index set such as , and random field is a random function on any set (typically time, space, or a discrete set).

If a random variable defined on the probability space is given, we can ask questions like "How likely is it that the value of is equal to 2?". This is the same as the probability of the event which is often written as or for short.

Recording all these probabilities of outputs of a random variable yields the probability distribution of . The probability distribution "forgets" about the particular probability space used to define and only records the probabilities of various output values of . Such a probability distribution, if is real-valued, can always be captured by its cumulative distribution function

and sometimes also using a probability density function, . In measure-theoretic terms, we use the random variable to "push-forward" the measure on to a measure on . The measure is called the "(probability) distribution of " or the "law of ".
^{[8]} The density , the Radon–Nikodym derivative of with respect to some reference measure on (often, this reference measure is the Lebesgue measure in the case of continuous random variables, or the counting measure in the case of discrete random variables).
The underlying probability space is a technical device used to guarantee the existence of random variables, sometimes to construct them, and to define notions such as correlation and dependence or independence based on a joint distribution of two or more random variables on the same probability space. In practice, one often disposes of the space altogether and just puts a measure on that assigns measure 1 to the whole real line, i.e., one works with probability distributions instead of random variables. See the article on quantile functions for fuller development.

In an experiment a person may be chosen at random, and one random variable may be the person's height. Mathematically, the random variable is interpreted as a function which maps the person to the person's height. Associated with the random variable is a probability distribution that allows the computation of the probability that the height is in any subset of possible values, such as the probability that the height is between 180 and 190 cm, or the probability that the height is either less than 150 or more than 200 cm.

Another random variable may be the person's number of children; this is a discrete random variable with non-negative integer values. It allows the computation of probabilities for individual integer values – the probability mass function (PMF) – or for sets of values, including infinite sets. For example, the event of interest may be "an even number of children". For both finite and infinite event sets, their probabilities can be found by adding up the PMFs of the elements; that is, the probability of an even number of children is the infinite sum .

In examples such as these, the sample space is often suppressed, since it is mathematically hard to describe, and the possible values of the random variables are then treated as a sample space. But when two random variables are measured on the same sample space of outcomes, such as the height and number of children being computed on the same random persons, it is easier to track their relationship if it is acknowledged that both height and number of children come from the same random person, for example so that questions of whether such random variables are correlated or not can be posed.

If are countable sets of real numbers, and , then is a discrete distribution function. Here for , for . Taking for instance an enumeration of all rational numbers as , one gets a discrete function that is not necessarily a step function (piecewise constant).

The possible outcomes for one coin toss can be described by the sample space . We can introduce a real-valued random variable that models a $1 payoff for a successful bet on heads as follows:

If the coin is a fair coin, *Y* has a probability mass function given by:

A random variable can also be used to describe the process of rolling dice and the possible outcomes. The most obvious representation for the two-dice case is to take the set of pairs of numbers *n*_{1} and *n*_{2} from {1, 2, 3, 4, 5, 6} (representing the numbers on the two dice) as the sample space. The total number rolled (the sum of the numbers in each pair) is then a random variable *X* given by the function that maps the pair to the sum:

Formally, a continuous random variable is a random variable whose cumulative distribution function is continuous everywhere.^{[9]} There are no "gaps", which would correspond to numbers which have a finite probability of occurring. Instead, continuous random variables almost never take an exact prescribed value *c* (formally, ) but there is a positive probability that its value will lie in particular intervals which can be arbitrarily small. Continuous random variables usually admit probability density functions (PDF), which characterize their CDF and probability measures;
such distributions are also called absolutely continuous; but some continuous distributions are singular, or mixes of an absolutely continuous part and a singular part.

An example of a continuous random variable would be one based on a spinner that can choose a horizontal direction. Then the values taken by the random variable are directions. We could represent these directions by North, West, East, South, Southeast, etc. However, it is commonly more convenient to map the sample space to a random variable which takes values which are real numbers. This can be done, for example, by mapping a direction to a bearing in degrees clockwise from North. The random variable then takes values which are real numbers from the interval [0, 360), with all parts of the range being "equally likely". In this case, * X* = the angle spun. Any real number has probability zero of being selected, but a positive probability can be assigned to any

More formally, given any interval , a random variable is called a "continuous uniform random variable" (CURV) if the probability that it takes a value in a subinterval depends only on the length of the subinterval. This implies that the probability of falling in any subinterval is proportional to the length of the subinterval, that is, if *a* ≤ *c* ≤ *d* ≤ *b*, one has

where the last equality results from the unitarity axiom of probability. The probability density function of a CURV is given by the indicator function of its interval of support normalized by the interval's length:

A **mixed random variable** is a random variable whose cumulative distribution function is neither discrete nor everywhere-continuous.^{[9]} It can be realized as a mixture of a discrete random variable and a continuous random variable; in which case the CDF will be the weighted average of the CDFs of the component variables.^{[9]}

An example of a random variable of mixed type would be based on an experiment where a coin is flipped and the spinner is spun only if the result of the coin toss is heads. If the result is tails, * X* = −1; otherwise

Most generally, every probability distribution on the real line is a mixture of discrete part, singular part, and an absolutely continuous part; see Lebesgue's decomposition theorem § Refinement. The discrete part is concentrated on a countable set, but this set may be dense (like the set of all rational numbers).

The most formal, axiomatic definition of a random variable involves measure theory. Continuous random variables are defined in terms of sets of numbers, along with functions that map such sets to probabilities. Because of various difficulties (e.g. the Banach–Tarski paradox) that arise if such sets are insufficiently constrained, it is necessary to introduce what is termed a sigma-algebra to constrain the possible sets over which probabilities can be defined. Normally, a particular such sigma-algebra is used, the Borel σ-algebra, which allows for probabilities to be defined over any sets that can be derived either directly from continuous intervals of numbers or by a finite or countably infinite number of unions and/or intersections of such intervals.^{[10]}

The measure-theoretic definition is as follows.

Let be a probability space and a measurable space. Then an ** -valued random variable** is a measurable function , which means that, for every subset , its preimage is -measurable; , where .^{[11]} This definition enables us to measure any subset in the target space by looking at its preimage, which by assumption is measurable.

In more intuitive terms, a member of is a possible outcome, a member of is a measurable subset of possible outcomes, the function gives the probability of each such measurable subset, represents the set of values that the random variable can take (such as the set of real numbers), and a member of is a "well-behaved" (measurable) subset of (those for which the probability may be determined). The random variable is then a function from any outcome to a quantity, such that the outcomes leading to any useful subset of quantities for the random variable have a well-defined probability.

When is a topological space, then the most common choice for the σ-algebra is the Borel σ-algebra , which is the σ-algebra generated by the collection of all open sets in . In such case the -valued random variable is called an ** -valued random variable**. Moreover, when the space is the real line , then such a real-valued random variable is called simply a **random variable**.

In this case the observation space is the set of real numbers. Recall, is the probability space. For a real observation space, the function is a real-valued random variable if

This definition is a special case of the above because the set generates the Borel σ-algebra on the set of real numbers, and it suffices to check measurability on any generating set. Here we can prove measurability on this generating set by using the fact that .

The probability distribution of a random variable is often characterised by a small number of parameters, which also have a practical interpretation. For example, it is often enough to know what its "average value" is. This is captured by the mathematical concept of expected value of a random variable, denoted , and also called the **first moment.** In general, is not equal to . Once the "average value" is known, one could then ask how far from this average value the values of typically are, a question that is answered by the variance and standard deviation of a random variable. can be viewed intuitively as an average obtained from an infinite population, the members of which are particular evaluations of .

Mathematically, this is known as the (generalised) problem of moments: for a given class of random variables , find a collection of functions such that the expectation values fully characterise the distribution of the random variable .

Moments can only be defined for real-valued functions of random variables (or complex-valued, etc.). If the random variable is itself real-valued, then moments of the variable itself can be taken, which are equivalent to moments of the identity function of the random variable. However, even for non-real-valued random variables, moments can be taken of real-valued functions of those variables. For example, for a categorical random variable *X* that can take on the nominal values "red", "blue" or "green", the real-valued function can be constructed; this uses the Iverson bracket, and has the value 1 if has the value "green", 0 otherwise. Then, the expected value and other moments of this function can be determined.

A new random variable *Y* can be defined by applying a real Borel measurable function to the outcomes of a real-valued random variable . That is, . The cumulative distribution function of is then

If function is invertible (i.e., exists, where is 's inverse function) and is either increasing or decreasing, then the previous relation can be extended to obtain

With the same hypotheses of invertibility of , assuming also differentiability, the relation between the probability density functions can be found by differentiating both sides of the above expression with respect to , in order to obtain^{[9]}

If there is no invertibility of but each admits at most a countable number of roots (i.e., a finite, or countably infinite, number of such that ) then the previous relation between the probability density functions can be generalized with

where , according to the inverse function theorem. The formulas for densities do not demand to be increasing.

In the measure-theoretic, axiomatic approach to probability, if a random variable on and a Borel measurable function , then is also a random variable on , since the composition of measurable functions is also measurable. (However, this is not necessarily true if is Lebesgue measurable.^{[citation needed]}) The same procedure that allowed one to go from a probability space to can be used to obtain the distribution of .

Let be a real-valued, continuous random variable and let .

If , then , so

If , then

so

Suppose is a random variable with a cumulative distribution

where is a fixed parameter. Consider the random variable Then,

The last expression can be calculated in terms of the cumulative distribution of so

which is the cumulative distribution function (CDF) of an exponential distribution.

Suppose is a random variable with a standard normal distribution, whose density is

Consider the random variable We can find the density using the above formula for a change of variables:

In this case the change is not monotonic, because every value of has two corresponding values of (one positive and negative). However, because of symmetry, both halves will transform identically, i.e.,

The inverse transformation is

and its derivative is

Then,

This is a chi-squared distribution with one degree of freedom.

Suppose is a random variable with a normal distribution, whose density is

Consider the random variable We can find the density using the above formula for a change of variables:

In this case the change is not monotonic, because every value of has two corresponding values of (one positive and negative). Differently from the previous example, in this case however, there is no symmetry and we have to compute the two distinct terms:

The inverse transformation is

and its derivative is

Then,

This is a noncentral chi-squared distribution with one degree of freedom.

- The probability distribution of the sum of two independent random variables is the
**convolution**of each of their distributions. - Probability distributions are not a vector space—they are not closed under linear combinations, as these do not preserve non-negativity or total integral 1—but they are closed under convex combination, thus forming a convex subset of the space of functions (or measures).

There are several different senses in which random variables can be considered to be equivalent. Two random variables can be equal, equal almost surely, or equal in distribution.

In increasing order of strength, the precise definition of these notions of equivalence is given below.

If the sample space is a subset of the real line, random variables *X* and *Y* are *equal in distribution* (denoted ) if they have the same distribution functions:

To be equal in distribution, random variables need not be defined on the same probability space. Two random variables having equal moment generating functions have the same distribution. This provides, for example, a useful method of checking equality of certain functions of independent, identically distributed (IID) random variables. However, the moment generating function exists only for distributions that have a defined Laplace transform.

Two random variables *X* and *Y* are *equal almost surely* (denoted ) if, and only if, the probability that they are different is zero:

For all practical purposes in probability theory, this notion of equivalence is as strong as actual equality. It is associated to the following distance:

where "ess sup" represents the essential supremum in the sense of measure theory.

Finally, the two random variables *X* and *Y* are *equal* if they are equal as functions on their measurable space:

This notion is typically the least useful in probability theory because in practice and in theory, the underlying measure space of the experiment is rarely explicitly characterized or even characterizable.

A significant theme in mathematical statistics consists of obtaining convergence results for certain sequences of random variables; for instance the law of large numbers and the central limit theorem.

There are various senses in which a sequence of random variables can converge to a random variable . These are explained in the article on convergence of random variables.

- Aleatoricism
- Algebra of random variables
- Event (probability theory)
- Multivariate random variable
- Pairwise independent random variables
- Observable variable
- Random element
- Random function
- Random measure
- Random number generator produces a random value
- Random variate
- Random vector
- Randomness
- Stochastic process
- Relationships among probability distributions

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