Random variables and distributions

Part of Probability · 27 questions on this topic · What links here

A random variable is a numerical summary of an experiment. Once the sample space and the probability are fixed, the distribution of that summary is enough for any question that depends on the experiment only through the summary. Means, variances and the named families on the common distributions page are all statements about such summaries. This chapter says which experiment produces which family. The sheet records the probability function, the mean and the variance in the parameterisation used here. The second gamma parameter on that sheet is a rate. The geometric law there starts at 1.

Two families are not on the sheet, so their formulas are written out below: the uniform distribution on an interval, and the hypergeometric distribution.

Random variables

Definition 1 (Random variable) A random variable is a function X from the sample space \Omega to the real numbers. The event \{X\le x\} is the set of outcomes \omega with X(\omega)\le x.

Article: Random variable →

Two dice have sample space \{1,\ldots,6\}^2. Their sum X(i,j)=i+j is a random variable with values in \{2,\ldots,12\}. The number of heads in n coin tosses is a random variable on \{0,1\}^n. The modelling gain is that later calculations can ignore the underlying outcomes and work with X alone.

Definition 2 (Cumulative distribution function) The cumulative distribution function of X is F(x)=\mathbb{P}(X\le x), for x\in\mathbb{R}.

Article: Cumulative distribution function →

Every distribution function is non-decreasing, tends to 0 as x\to-\infty and to 1 as x\to\infty, and is right-continuous. Conversely, any function with those properties is the distribution function of some random variable. For a<b,

\mathbb{P}(a<X\le b)=F(b)-F(a).

Definition 3 (Discrete distribution) X is discrete when it takes values in a countable set S. Its probability mass function is f(x)=\mathbb{P}(X=x) for x\in S, and \mathbb{P}(X\in B)=\sum_{x\in B}f(x).

Article: Discrete distribution →

A fair die has mass function f(x)=1/6 on \{1,\ldots,6\}. The mass function determines the distribution function by adding the atoms up to x, and the jumps of the distribution function are the atoms.

Definition 4 (Continuous distribution) X is continuous when its distribution function can be written F(x)=\int_{-\infty}^{x} f(u)\,\,\mathrm{d} u for a non-negative function f with \int_{-\infty}^{\infty} f=1. The function f is a probability density. Then \mathbb{P}(X\in B)=\int_B f, and f=F' at every point where F is differentiable.

Article: Continuous distribution →

A density is not a probability. The probability of an infinitesimal interval (x,x+\,\mathrm{d} x) is about f(x)\,\,\mathrm{d} x. A single point still has probability zero. Drawing uniformly from [0,1] has density f(x)=1 on that interval and distribution function F(x)=x there.

Figure 1: Mass, density and distribution function. Left: a fair die’s mass function, and its distribution function, a right-continuous staircase whose jumps are the masses. Right: an \operatorname{Exp}(1) density, with \mathbb{P}(0.5<X\le1.6) as the area under it, and the same probability as the rise F(1.6)-F(0.5) of the distribution function.

Expectation and variance

Definition 5 (Expectation) If X is discrete with mass function f, its expectation is \mathbb{E} X=\sum_x x\,f(x), when the sum converges absolutely. If X is continuous with density f, \mathbb{E} X=\int_{-\infty}^{\infty} x\,f(x)\,\,\mathrm{d} x, when the integral converges absolutely.

Article: Expectation →

The expectation is a centre of mass: point masses f(x) placed at the positions x balance at \mathbb{E} X. A symmetric mass function therefore has expectation at the centre of symmetry, when the expectation exists. The expectation need not be a value that X can take. A fair die has expectation 7/2.

Theorem 1 (Expectation of a function) If g is a real function and X is discrete with mass function f, then \mathbb{E} g(X)=\sum_x g(x)\,f(x). If X is continuous with density f, then \mathbb{E} g(X)=\int_{-\infty}^{\infty} g(x)\,f(x)\,\,\mathrm{d} x, whenever the sum or integral converges absolutely.

In the discrete case, group the outcomes on which g takes the value y. The mass at y is \sum_{x:g(x)=y}f(x), so \mathbb{E} g(X)=\sum_y y\sum_{x:g(x)=y}f(x)=\sum_x g(x)\,f(x).

Article: Expectation of a function →

Linearity is the useful consequence. For constants a and b, and functions g and h whose expectations exist,

\mathbb{E}(aX+b)=a\,\mathbb{E} X+b, \qquad \mathbb{E}\bigl(g(X)+h(X)\bigr)=\mathbb{E} g(X)+\mathbb{E} h(X).

No independence is required. Linearity is why a sum of indicators has expectation equal to the sum of the probabilities, even when the indicators are dependent.

Definition 6 (Variance) The variance of X is \operatorname{Var}(X)=\mathbb{E}(X-\mathbb{E} X)^2, when that expectation exists. Equivalently, \operatorname{Var}(X)=\mathbb{E} X^2-(\mathbb{E} X)^2. The standard deviation is the square root of the variance.

Article: Variance →

Variance measures spread about the expectation. It scales by the square of a constant: \operatorname{Var}(aX+b)=a^2\operatorname{Var}(X). The shift b does not appear, because variance ignores location.

Transforms

Definition 7 (Probability generating function) If N takes values in \{0,1,2,\ldots\}, its probability generating function is G(z)=\mathbb{E} z^N=\sum_{n=0}^{\infty}\mathbb{P}(N=n)\,z^n, for |z|\le 1.

Article: Probability generating function →

The mass function can be recovered by differentiation at the origin: \mathbb{P}(N=n)=G^{(n)}(0)/n!. The mean and variance sit at the other endpoint, when they exist:

\mathbb{E} N=G'(1), \qquad \operatorname{Var}(N)=G''(1)+G'(1)-\bigl(G'(1)\bigr)^2.

For a fair comparison with the sheet, the generating functions of the named non-negative integer laws are (1-p+zp) for a Bernoulli trial, (1-p+zp)^n for a binomial count, zp/(1-(1-p)z) for a geometric count that starts at 1, and e^{\lambda(z-1)} for a Poisson count.

Definition 8 (Moment generating function) The moment generating function of X is M(s)=\mathbb{E} e^{sX}, for those s at which the expectation exists.

Article: Moment generating function →

If M exists in an open interval around 0, it determines the distribution, and the moments are derivatives at the origin: \mathbb{E} X^n=M^{(n)}(0). The practical use is addition. If X and Y are independent, then M_{X+Y}(s)=M_X(s)M_Y(s) wherever both factors exist. That is often the shortest proof that a sum stays inside a family.

Named distributions

A handful of distributions recur because a handful of experiments recur. Each is listed with the experiment it describes, and its mean and variance are derived from the generating functions above, so the formulas on the common distributions page can be rebuilt rather than memorised.

Figure 2: Three discrete laws: the number of successes in 10 trials with success probability 0.7, the trial of the first success when each trial succeeds with probability 0.3, and a Poisson count with mean 10.

Bernoulli and binomial

Definition 9 (Bernoulli distribution) X has the Bernoulli distribution with success probability p\in[0,1], written X\sim\operatorname{Bern}(p), when \mathbb{P}(X=1)=p and \mathbb{P}(X=0)=1-p. Then \mathbb{E} X=p and \operatorname{Var}(X)=p(1-p).

Article: Bernoulli distribution →

A Bernoulli variable records a single trial: success as 1, failure as 0. Because X^2=X, \mathbb{E} X^2=p and \operatorname{Var}(X)=p-p^2. The variance is largest, 1/4, at p=1/2, where the outcome is least predictable.

Definition 10 (Binomial distribution) X has the binomial distribution with n trials and success probability p, written X\sim\operatorname{Bin}(n,p), when

\mathbb{P}(X=x)=\binom nx p^x(1-p)^{n-x},\qquad x=0,1,\ldots,n.

It is the number of successes in n independent \operatorname{Bern}(p) trials. Then \mathbb{E} X=np and \operatorname{Var}(X)=np(1-p).

Article: Binomial distribution →

The mass function is the coin-toss count of Random experiments and probability: each sequence with x successes has probability p^x(1-p)^{n-x}, and there are \binom nx of them. The moments are quickest from the generating function. Writing X=X_1+\cdots+X_n for the n independent trials, each with generating function 1-p+pz,

G(z)=(1-p+pz)^n,\qquad G'(1)=np,\qquad G''(1)=n(n-1)p^2,

so \mathbb{E} X=np and \operatorname{Var}(X)=n(n-1)p^2+np-n^2p^2=np(1-p). The same answer follows without generating functions: the mean of a sum is the sum of the means, and the variance of a sum of independent terms is the sum of the variances.

Example 1 (Defective items in a box) Each item from a production line is defective with probability 0.05, independently of the others. A box holds 20 items.

Question. Find the expected number of defective items in a box, and the probability that a box has at most one.

Solution. The number of defectives is X\sim\operatorname{Bin}(20,0.05), so \mathbb{E} X=20\times0.05=1. Then

\mathbb{P}(X\le1)=0.95^{20}+20\times0.05\times0.95^{19}=0.358+0.377=0.736.

Although the average is exactly one defective, more than a quarter of boxes have two or more.

Geometric

Definition 11 (Geometric distribution) X has the geometric distribution with success probability p\in(0,1], written X\sim\operatorname{Geom}(p), when

\mathbb{P}(X=x)=(1-p)^{x-1}p,\qquad x=1,2,\ldots

It is the trial on which the first success occurs, in a sequence of independent \operatorname{Bern}(p) trials. Then \mathbb{E} X=1/p and \operatorname{Var}(X)=(1-p)/p^2.

Article: Geometric distribution →

The first success is at trial x exactly when the first x-1 trials fail and trial x succeeds, which gives the mass function, and \mathbb{P}(X>x)=(1-p)^x because that happens when the first x trials fail. With q=1-p the generating function is a geometric series,

G(z)=\sum_{x=1}^\infty q^{x-1}p\,z^x=\frac{pz}{1-qz},\qquad G'(z)=\frac{p}{(1-qz)^2},\qquad G''(z)=\frac{2pq}{(1-qz)^3}.

So \mathbb{E} X=G'(1)=1/p and \operatorname{Var}(X)=2q/p^2+1/p-1/p^2=q/p^2. A fair die needs six throws on average to show its first six. Some books count the failures before the first success instead, X-1, which has mean (1-p)/p; the two conventions differ by exactly one.

Poisson

Definition 12 (Poisson distribution) X has the Poisson distribution with mean \lambda>0, written X\sim\operatorname{Poisson}(\lambda), when

\mathbb{P}(X=x)=e^{-\lambda}\frac{\lambda^x}{x!},\qquad x=0,1,2,\ldots

Then \mathbb{E} X=\operatorname{Var}(X)=\lambda.

Article: Poisson distribution →

Theorem 2 (Poisson limit of the binomial) If X_n\sim\operatorname{Bin}(n,p_n) with np_n\to\lambda as n\to\infty, then \mathbb{P}(X_n=x)\to e^{-\lambda}\lambda^x/x! for every x=0,1,2,\ldots

Article: Poisson limit of the binomial →

Write p_n=\lambda_n/n with \lambda_n\to\lambda. Then

\binom nx p_n^x(1-p_n)^{n-x}=\frac{\lambda_n^x}{x!}\cdot\frac{n(n-1)\cdots(n-x+1)}{n^x}\cdot\Bigl(1-\frac{\lambda_n}n\Bigr)^n\Bigl(1-\frac{\lambda_n}n\Bigr)^{-x}.

As n\to\infty the second factor tends to 1, the third to e^{-\lambda} and the fourth to 1. That is why the Poisson law models the number of rare events in a fixed interval of time or space: many independent chances, each small, with a steady average number of successes. Calls to an exchange, decays of a radioactive sample and typing errors on a page are the standard examples.

The generating function is G(z)=\sum_x e^{-\lambda}(\lambda z)^x/x!=e^{\lambda(z-1)}. Then G'(1)=\lambda and G''(1)=\lambda^2, so the mean is \lambda and the variance is \lambda^2+\lambda-\lambda^2=\lambda. Equal mean and variance is the signature of a Poisson count, and data whose variance is well above the mean are called overdispersed; see Standard errors, and models for counts.

Example 2 (A rare fault) A machine makes 1000 parts a day, and each part has a fault with probability 0.002, independently.

Question. Find the probability that a day has at most one faulty part, exactly and by the Poisson approximation.

Solution. The exact count is \operatorname{Bin}(1000,0.002), and \mathbb{P}(X\le1)=0.998^{1000}+1000\times0.002\times0.998^{999}=0.4057. The Poisson approximation uses \lambda=1000\times0.002=2:

\mathbb{P}(X\le1)\approx e^{-2}(1+2)=0.4060.

The two agree to three decimal places. The approximation is good whenever n is large and p is small, and it needs only the product np.

Hypergeometric

Definition 13 (Hypergeometric distribution) A hypergeometric count draws n items without replacement from a population of size N that contains r marked items. If X is the number of marked items in the draw, then

\mathbb{P}(X=x)=\frac{\binom{r}{x}\binom{N-r}{n-x}}{\binom{N}{n}},

for every integer x with \max(0,n-(N-r))\le x\le\min(n,r). Write p=r/N. Then \mathbb{E} X=np and

\operatorname{Var}(X)=np(1-p)\frac{N-n}{N-1}.

Article: Hypergeometric distribution →

The mass function counts the ways to choose x of the marked items and n-x of the others, over the ways to choose any n. The mean matches the with-replacement, binomial, experiment. The variance is smaller by the factor (N-n)/(N-1), which is the effect of not putting items back. When the population is much larger than the sample, the factor is close to 1 and the binomial is a good approximation.

Example 3 (Aces in a hand) Five cards are dealt from a well-shuffled deck of 52.

Question. Find the distribution of the number of aces, and compare it with the binomial count for five draws with replacement.

Solution. The number of aces is hypergeometric with N=52, r=4 and n=5. For example,

\mathbb{P}(X=1)=\frac{\binom41\binom{48}4}{\binom{52}5}=\frac{4\times194580}{2598960}=0.2995.

The full distribution is 0.6588, 0.2995, 0.0399, 0.0017 and 0.00002 for 0 to 4 aces. The binomial count \operatorname{Bin}(5,1/13) gives 0.6702, 0.2792 and 0.0465 for 0 to 2. Both have mean 5/13=0.385, but without replacement each ace drawn makes the next less likely, so the hypergeometric count is less spread out.

Uniform

Definition 14 (Uniform distribution) X is uniform on the interval [a,b], written X\sim\operatorname{U}[a,b], when its density is 1/(b-a) on that interval and zero elsewhere. Then \mathbb{E} X=(a+b)/2 and \operatorname{Var}(X)=(b-a)^2/12.

Article: Uniform distribution →

The continuous analogue of an equally likely finite set is the uniform distribution: probability is proportional to length. The distribution function rises linearly from 0 to 1 across [a,b]. For the moments, \mathbb{E} X^2=\int_a^bx^2\,\,\mathrm{d} x/(b-a)=(a^2+ab+b^2)/3, and subtracting ((a+b)/2)^2 leaves (b-a)^2/12. The uniform law on [0,1] is the raw material of simulation.

Exponential

Definition 15 (Exponential distribution) X has the exponential distribution with rate \lambda>0, written X\sim\operatorname{Exp}(\lambda), when its density is \lambda e^{-\lambda x} for x>0. Its distribution function is 1-e^{-\lambda x}, its mean is 1/\lambda and its variance is 1/\lambda^2.

Article: Exponential distribution →

The moment generating function is M(s)=\int_0^\infty e^{sx}\lambda e^{-\lambda x}\,\mathrm{d} x=\lambda/(\lambda-s) for s<\lambda. Then M'(0)=1/\lambda and M''(0)=2/\lambda^2, so the variance is 2/\lambda^2-1/\lambda^2=1/\lambda^2. The exponential law is the usual model for a waiting time that does not age, and its defining property is the next theorem.

Theorem 3 (Memoryless property) A positive random variable X is memoryless when \mathbb{P}(X>s+t\mid X>s)=\mathbb{P}(X>t) for all s,t>0. The exponential distributions are the continuous memoryless laws, and the geometric distributions are the discrete ones.

For the exponential law with rate \lambda, the survival probability is e^{-\lambda x}, so

\mathbb{P}(X>s+t\mid X>s)=\frac{e^{-\lambda(s+t)}}{e^{-\lambda s}}=e^{-\lambda t}.

The geometric calculation is the same with (1-p)^{s+t} in place of e^{-\lambda(s+t)}.

Article: Memoryless property →

Memorylessness is a modelling claim. A component whose lifetime is exponential does not become more likely to fail as it gets older. The failure rate is constant. A bulb with exponential lifetime of mean 1000 hours that has already burned for 1000 hours survives another 500 with probability e^{-500/1000}=0.607, the same as a new bulb. Lifetime models that do age are on the reliability page.

Normal

Definition 16 (Normal distribution) X has the normal distribution with mean \mu and variance \sigma^2>0, written X\sim\operatorname{N}(\mu,\sigma^2), when its density is

\frac1{\sigma\sqrt{2\pi}}\exp\Bigl\{-\frac{(x-\mu)^2}{2\sigma^2}\Bigr\},\qquad x\in\mathbb{R}.

The standard normal distribution is \operatorname{N}(0,1), with distribution function written \Phi.

Article: Normal distribution →

The density is a bell centred at \mu, with inflection points at \mu\pm\sigma. An affine image of a normal variable is normal: if X\sim\operatorname{N}(\mu,\sigma^2) and a\ne 0, then aX+b\sim\operatorname{N}(a\mu+b,a^2\sigma^2). The moment generating function M(s)=\exp(\mu s+\sigma^2 s^2/2) makes this immediate, and it is proved again from the transformation rule in Functions of random variables and limit theorems.

The practical consequence is standardisation. If X\sim\operatorname{N}(\mu,\sigma^2) then Z=(X-\mu)/\sigma is standard normal, so every normal probability is a value of \Phi:

\mathbb{P}(a<X\le b)=\Phi\Bigl(\frac{b-\mu}\sigma\Bigr)-\Phi\Bigl(\frac{a-\mu}\sigma\Bigr).

By symmetry \Phi(-z)=1-\Phi(z), so tables list only z\ge0. A normal variable falls within one standard deviation of its mean with probability 0.683, within two with probability 0.954, and within three with probability 0.997.

Example 4 (IQ scores) Suppose IQ scores are \operatorname{N}(100,16^2).

Question. What fraction of people score between 90 and 110, and what fraction above 130?

Solution. Standardise: (90-100)/16=-0.625 and (110-100)/16=0.625, so

\mathbb{P}(90<X\le110)=\Phi(0.625)-\Phi(-0.625)=2\Phi(0.625)-1=0.468.

Above 130, z=1.875 and \mathbb{P}(X>130)=1-\Phi(1.875)=0.030, about one person in 33. These are the class probabilities used to sort recruits in Chi-squared tests.

Figure 3: Densities of three exponential laws, with rates 0.5, 1 and 2, and of three normal laws. The normal curves with standard deviations 0.5, 1 and 2 share a mean; the widest is the flattest because each must enclose area one.

Gamma and chi-squared

Definition 17 (Gamma distribution) X has the gamma distribution with shape \alpha>0 and rate \lambda>0, written X\sim\operatorname{Gamma}(\alpha,\lambda), when its density is

\frac{\lambda^\alpha x^{\alpha-1}e^{-\lambda x}}{\Gamma(\alpha)},\qquad x>0,

where \Gamma(\alpha)=\int_0^\infty u^{\alpha-1}e^{-u}\,\mathrm{d} u. Then \mathbb{E} X=\alpha/\lambda and \operatorname{Var}(X)=\alpha/\lambda^2.

Article: Gamma distribution →

Integration by parts gives \Gamma(\alpha+1)=\alpha\Gamma(\alpha), and \Gamma(1)=1, so \Gamma(k)=(k-1)! for whole numbers k; also \Gamma(1/2)=\sqrt\pi. The exponential law is the gamma law with shape 1. The moment generating function is M(s)=(\lambda/(\lambda-s))^\alpha for s<\lambda, so independent gamma variables with a common rate add their shapes. In particular, a sum of k independent \operatorname{Exp}(\lambda) waiting times is \operatorname{Gamma}(k,\lambda), the time of the kth event. A chi-squared variable with k degrees of freedom, used throughout Statistical inference, is the gamma law with shape k/2 and rate 1/2.

The time S_k of the kth event is longer than t exactly when fewer than k events have happened by time t. With events arriving at rate \lambda, that count is \operatorname{Poisson}(\lambda t), so

\mathbb{P}(S_k>t)=\sum_{j=0}^{k-1}e^{-\lambda t}\frac{(\lambda t)^j}{j!}.

For three events at rate 2 per hour, the probability that the third takes more than 2 hours is e^{-4}(1+4+8)=0.238.

Key idea

The distribution is the probability of the events \{X\in B\}. Discrete distributions are specified by a mass function, continuous distributions by a density. The expectation of a function is the average of that function against the mass or the density, and linearity does not need independence.

Questions on this topic

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