Continuous Random Variables
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Normal Distribution

The Normal (Gaussian) Distribution

The normal distribution is the most important continuous distribution in probability and statistics. Its PDF is:

fX(x)=1σ2πe−(x−μ)22σ2f_X(x) = \frac{1}{\sigma\sqrt{2\pi}} e^{-\frac{(x-\mu)^2}{2\sigma^2}}

Parameters

  • μ\mu = mean (center of the distribution)
  • σ\sigma = standard deviation (spread of the distribution)

Notation

We write X∼N(μ,σ2)X \sim N(\mu, \sigma^2) to indicate XX follows a normal distribution with mean μ\mu and variance σ2\sigma^2.


Properties

Shape

  • Symmetric around the mean μ\mu
  • Bell-shaped curve
  • The peak is at x=μx = \mu
  • The curve approaches 0 as x→±∞x \to \pm\infty

Spread

  • About 68% of values fall within μ±σ\mu \pm \sigma
  • About 95% of values fall within μ±2σ\mu \pm 2\sigma
  • About 99.7% of values fall within μ±3σ\mu \pm 3\sigma

This is the empirical rule or 68-95-99.7 rule.


Standard Normal Distribution

The standard normal has μ=0\mu = 0 and σ=1\sigma = 1:

ϕ(z)=12πe−z2/2\phi(z) = \frac{1}{\sqrt{2\pi}} e^{-z^2/2}

We use ZZ to denote a standard normal random variable.

Standardization

Any normal X∼N(μ,σ2)X \sim N(\mu, \sigma^2) can be converted to standard normal:

Z=X−μσZ = \frac{X - \mu}{\sigma}

Then Z∼N(0,1)Z \sim N(0, 1).


Cumulative Distribution Function

The CDF of the standard normal is denoted Φ(z)\Phi(z):

Φ(z)=P(Z≤z)=∫−∞zϕ(t) dt\Phi(z) = P(Z \leq z) = \int_{-\infty}^z \phi(t) \, dt

Properties

  • Φ(0)=0.5\Phi(0) = 0.5 (by symmetry)
  • Φ(−z)=1−Φ(z)\Phi(-z) = 1 - \Phi(z)
  • Values are tabulated or computed numerically (no closed form)

Why Is Normal Distribution Important?

Central Limit Theorem

The sum (or average) of many independent random variables tends to be normally distributed, regardless of the original distribution.

Natural Phenomena

Many natural measurements are approximately normal:

  • Heights, weights
  • Measurement errors
  • Test scores
  • Physical quantities

Statistical Inference

Many statistical methods assume normality:

  • Confidence intervals
  • Hypothesis tests
  • Regression analysis

Calculating Probabilities

Example: Finding P(a≤X≤b)P(a \leq X \leq b)

For X∼N(μ,σ2)X \sim N(\mu, \sigma^2):

  1. Standardize: Z=X−μσZ = \frac{X - \mu}{\sigma}
  2. Convert bounds: za=a−μσz_a = \frac{a - \mu}{\sigma}, zb=b−μσz_b = \frac{b - \mu}{\sigma}
  3. Use standard normal table or calculator:

    P(a≤X≤b)=Φ(zb)−Φ(za)P(a \leq X \leq b) = \Phi(z_b) - \Phi(z_a)

Example

For X∼N(100,152)X \sim N(100, 15^2), find P(85≤X≤115)P(85 \leq X \leq 115):

  1. z1=85−10015=−1z_1 = \frac{85 - 100}{15} = -1
  2. z2=115−10015=1z_2 = \frac{115 - 100}{15} = 1
  3. P(−1≤Z≤1)=Φ(1)−Φ(−1)=0.8413−0.1587=0.6826P(-1 \leq Z \leq 1) = \Phi(1) - \Phi(-1) = 0.8413 - 0.1587 = 0.6826

About 68% of values fall within one standard deviation of the mean.


Key Terms

Standard NormalA normal distribution with mean 0 and standard deviation 1; any normal can be standardized via Z = (X−μ)/σ.
StandardizationConverting a normal variable X to Z = (X−μ)/σ, yielding a standard normal distribution.
Empirical RuleFor a normal distribution: ~68% within 1σ, ~95% within 2σ, ~99.7% within 3σ of the mean.
Central Limit TheoremThe sum (or mean) of many independent random variables is approximately normal, regardless of their individual distributions.