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Standard Normal Distribution

Definition

A random variable ZZ has the standard normal distribution, written Z∼N(0,1)Z\sim\mathcal{N}(0,1), if its density is ϕ\phi; its CDF is Φ\Phi:

ϕ(z)=12πe−z2/2,Φ(z)=∫−∞zϕ(t) dt.\phi(z)=\frac{1}{\sqrt{2\pi}}\mathrm{e}^{-z^2/2},\qquad \Phi(z)=\int_{-\infty}^z\phi(t)\,\mathrm{d}t.

In N(μ,σ2)\mathcal{N}(\mu,\sigma^2) the second parameter is the variance.


Interpretation

The standard normal distribution is the single reference bell curve, centred at 00 with variance 11. Every normal probability can be read from its CDF Φ\Phi, because any normal variable becomes standard normal after standardization: a value is then measured in standard deviations from the mean.

The standard normal density with the area to the left of z = 1 shaded, equal to about 0.841.

The shaded area is everything to the left of z=1z=1, that is Φ(1)=P(Z≤1)≈0.841\Phi(1)=\mathbb{P}(Z\le1)\approx0.841, the first Example. The unshaded right tail has area 1−Φ(1)≈0.1591-\Phi(1)\approx0.159. Since ϕ\phi is symmetric about 00, the left tail below −1-1 has the same area, so Φ(−1)=1−Φ(1)\Phi(-1)=1-\Phi(1) and P(−1≤Z≤1)=2Φ(1)−1≈0.683\mathbb{P}(-1\le Z\le1)=2\Phi(1)-1\approx0.683.

Move cc and dd and read probabilities as differences Φ(d)−Φ(c)\Phi(d)-\Phi(c); try c=−1.96c=-1.96, d=1.96d=1.96.

The density ϕ\phi has no antiderivative in terms of elementary functions, so Φ\Phi is evaluated numerically, by a table or software. A table for z≥0z\ge0 suffices: symmetry gives Φ(−z)=1−Φ(z)\Phi(-z)=1-\Phi(z), and interval probabilities are differences Φ(d)−Φ(c)\Phi(d)-\Phi(c). The value 1.961.96 suggested in the manipulate prompt satisfies Φ(1.96)≈0.975\Phi(1.96)\approx0.975, so P(−1.96≤Z≤1.96)≈0.95\mathbb{P}(-1.96\le Z\le1.96)\approx0.95.

For Y∼N(μ,σ2)Y\sim\mathcal{N}(\mu,\sigma^2), the variable (Y−μ)/σ(Y-\mu)/\sigma is standard normal, so P(Y≤y)=Φ((y−μ)/σ)\mathbb{P}(Y\le y)=\Phi\big((y-\mu)/\sigma\big); the second Example uses this with μ=10\mu=10 and σ=2\sigma=2. A common slip is to divide by the variance: in N(10,4)\mathcal{N}(10,4) the second parameter is σ2=4\sigma^2=4, so the divisor is σ=2\sigma=2. Later, sums of many independent variables are approximated by this distribution after standardization, in the central limit theorem.


Key Results

  • EZ=0\mathbb{E}Z=0, Var⁡(Z)=1\operatorname{Var}(Z)=1, and Φ(−z)=1−Φ(z)\Phi(-z)=1-\Phi(z).
  • If Y∼N(μ,σ2)Y\sim\mathcal{N}(\mu,\sigma^2) with σ>0\sigma>0, then (Y−μ)/σ∼N(0,1)(Y-\mu)/\sigma\sim\mathcal{N}(0,1).
  • Quantiles transform the same way: the pp-quantile of YY is μ+σΦ−1(p)\mu+\sigma\Phi^{-1}(p). Printed normal tables list the left-tail probabilities Φ(z)\Phi(z), so a quantile is read off the table in reverse and then transformed back.

Examples

  • P(Z≤1)=Φ(1)≈0.8413\mathbb{P}(Z\le1)=\Phi(1)\approx0.8413.
  • For Y∼N(10,4)Y\sim\mathcal{N}(10,4), P(Y≤12)=Φ((12−10)/2)=Φ(1)≈0.8413\mathbb{P}(Y\le12)=\Phi((12-10)/2)=\Phi(1)\approx0.8413.

Prerequisites

Sources

Aliases: N(0,1), standard Gaussian, standard normal, unit normal distribution, standard normal random variable, standard Gaussian distribution Symbols: infinity, integral, mu, phi, pi, sigma, square root

Last updated: 22 October 2026 19:04