The Normal Distribution

The normal distribution is the famous bell curve — the smooth, symmetric hump that so many real-world measurements follow: heights, test scores, measurement errors, and much more. It is the single most important distribution in statistics.

A normal distribution is pinned down by just two numbers: its mean \mu and its standard deviation \sigma. We write

X \sim N(\mu, \sigma^2)

to say that X is normal with mean \mu and variance \sigma^2 (so standard deviation \sigma).

Centre and width

The two numbers play two very different roles:

The curve is perfectly symmetric about \mu, so for a normal distribution the mean, median, and mode all coincide — they sit together right at the peak.

The density formula

The height of the bell at each value x is given by its density:

f(x) = \frac{1}{\sigma\sqrt{2\pi}}\,\exp\!\left(-\frac{(x-\mu)^2}{2\sigma^2}\right).

You don't need to memorise this to use it — just notice that the value x only ever appears as (x-\mu)^2, the squared distance from the centre. That squared distance is why the curve falls away smoothly and symmetrically on both sides of \mu. As always, the total area under the curve is 1, so a narrower bell must rise taller to keep its area fixed.

(A deeper, measure-theoretic treatment of the same curve — standardisation, the Gaussian integral, and more — lives at the normal distribution in finance.)

Shape the bell

Slide \mu to move the curve, and \sigma to make it wider or narrower. The faint curve is the fixed standard normal N(0,1) for comparison. Watch how a narrower bell grows taller — the area underneath stays 1.