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Part IA Easter Term

Normal Distribution

Importance

The normal distribution (Gaussian) is the most important distribution in statistics. It appears naturally as the limit of sums (Central Limit Theorem) and models many physical phenomena.

Climate: heights, measurement errors, IQ scores, physical measurements, and economic data all approximate normal distributions.

Definition

XN(μ,σ2)X \sim N(\mu, \sigma^2) has PDF:

f(x)=1σ2πe(xμ)22σ2,xRf(x) = \frac{1}{\sigma\sqrt{2\pi}} e^{-\frac{(x-\mu)^2}{2\sigma^2}}, \quad x \in \mathbb{R}

Parameters

  • μ\mu: mean (centre)
  • σ2\sigma^2: variance (spread), σ>0\sigma > 0

Range

X(,)X \in (-\infty, \infty) (all real numbers)

CDF

F(x)=Φ(xμσ)F(x) = \Phi\left(\frac{x - \mu}{\sigma}\right)

where Φ\Phi is the CDF of the standard normal N(0,1)N(0,1). No closed form exists; we use tables or software.

Properties

Symmetry

The normal is symmetric around μ\mu:

P(Xμa)=P(Xμ+a)P(X \leq \mu - a) = P(X \geq \mu + a)

f(μ+a)=f(μa)f(\mu + a) = f(\mu - a)

Mean equals Median equals Mode

E[X]=μ=median=modeE[X] = \mu = \text{median} = \text{mode}

Variance

Var(X)=σ2\text{Var}(X) = \sigma^2

Linear Transformations

If XN(μ,σ2)X \sim N(\mu, \sigma^2) and Y=aX+bY = aX + b (a0a \neq 0):

YN(aμ+b,a2σ2)Y \sim N(a\mu + b, a^2\sigma^2)

Important: Any linear transformation of a normal is still normal.

Standard Normal

The standard normal ZN(0,1)Z \sim N(0, 1) has:

ϕ(z)=12πez2/2\phi(z) = \frac{1}{\sqrt{2\pi}} e^{-z^2/2}

CDF: Φ(z)=P(Zz)\Phi(z) = P(Z \leq z)

Standardisation

For XN(μ,σ2)X \sim N(\mu, \sigma^2):

Z=XμσN(0,1)Z = \frac{X - \mu}{\sigma} \sim N(0, 1)

This converts any normal to standard normal, enabling use of standard tables.

Visualisation

The normal PDF is the famous “bell curve”: symmetric, peaked at μ\mu, with spread controlled by σ\sigma.

  • μ\mu shifts the centre
  • σ\sigma controls the width: larger σ\sigma = more spread

Normal PDFs for different parameters

Probability Calculations

Use standardisation and Φ\Phi tables.

P(Xx)=Φ(xμσ)P(X \leq x) = \Phi\left(\frac{x - \mu}{\sigma}\right)

P(aXb)=Φ(bμσ)Φ(aμσ)P(a \leq X \leq b) = \Phi\left(\frac{b - \mu}{\sigma}\right) - \Phi\left(\frac{a - \mu}{\sigma}\right)

Example

XN(100,152)X \sim N(100, 15^2). Find P(X115)P(X \leq 115).

Standardise: Z=11510015=1Z = \frac{115 - 100}{15} = 1

P(X115)=P(Z1)=Φ(1)0.841P(X \leq 115) = P(Z \leq 1) = \Phi(1) \approx 0.841

From tables: Φ(1)0.8413\Phi(1) \approx 0.8413.

Empirical Rule (68-95-99.7)

For any normal N(μ,σ2)N(\mu, \sigma^2):

IntervalCoverage
μ±σ\mu \pm \sigma68%\approx 68\%
μ±2σ\mu \pm 2\sigma95%\approx 95\%
μ±3σ\mu \pm 3\sigma99.7%\approx 99.7\%

This is useful for quick estimates.

Exact Values

Φ(1)Φ(1)=0.84130.1587=0.6826\Phi(1) - \Phi(-1) = 0.8413 - 0.1587 = 0.6826

Φ(2)Φ(2)=0.97720.0228=0.9544\Phi(2) - \Phi(-2) = 0.9772 - 0.0228 = 0.9544

Φ(3)Φ(3)=0.99870.0013=0.9974\Phi(3) - \Phi(-3) = 0.9987 - 0.0013 = 0.9974

Sum of Independent Normals

If XN(μ1,σ12)X \sim N(\mu_1, \sigma_1^2) and YN(μ2,σ22)Y \sim N(\mu_2, \sigma_2^2) are independent:

X+YN(μ1+μ2,σ12+σ22)X + Y \sim N(\mu_1 + \mu_2, \sigma_1^2 + \sigma_2^2)

The sum of independent normals is normal. This is not true for arbitrary sums.

Extending to nn Variables

For independent XiN(μ,σ2)X_i \sim N(\mu, \sigma^2):

Xˉ=1nXiN(μ,σ2n)\bar{X} = \frac{1}{n}\sum X_i \sim N\left(\mu, \frac{\sigma^2}{n}\right)

Summary Table

PropertyValue
PDF1σ2πe(xμ)2/(2σ2)\frac{1}{\sigma\sqrt{2\pi}} e^{-(x-\mu)^2/(2\sigma^2)}
Meanμ\mu
Varianceσ2\sigma^2
Standard normalN(0,1)N(0, 1)
StandardisationZ=XμσZ = \frac{X - \mu}{\sigma}
Sum of independent normalsNormal with μ=μ1+μ2\mu = \mu_1 + \mu_2, σ2=σ12+σ22\sigma^2 = \sigma_1^2 + \sigma_2^2