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
X∼N(μ,σ2) has PDF:
f(x)=σ2π1e−2σ2(x−μ)2,x∈R
Parameters
μ: mean (centre)
σ2: variance (spread), σ>0
Range
X∈(−∞,∞) (all real numbers)
CDF
F(x)=Φ(σx−μ)
where Φ is the CDF of the standard normal N(0,1). No closed form exists; we use tables or software.
Properties
Symmetry
The normal is symmetric around μ:
P(X≤μ−a)=P(X≥μ+a)
f(μ+a)=f(μ−a)
Mean equals Median equals Mode
E[X]=μ=median=mode
Variance
Var(X)=σ2
Linear Transformations
If X∼N(μ,σ2) and Y=aX+b (a=0):
Y∼N(aμ+b,a2σ2)
Important: Any linear transformation of a normal is still normal.
Standard Normal
The standard normal Z∼N(0,1) has:
ϕ(z)=2π1e−z2/2
CDF: Φ(z)=P(Z≤z)
Standardisation
For X∼N(μ,σ2):
Z=σX−μ∼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, with spread controlled by σ.
μ shifts the centre
σ controls the width: larger σ = more spread
Probability Calculations
Use standardisation and Φ tables.
P(X≤x)=Φ(σx−μ)
P(a≤X≤b)=Φ(σb−μ)−Φ(σa−μ)
Example
X∼N(100,152). Find P(X≤115).
Standardise: Z=15115−100=1
P(X≤115)=P(Z≤1)=Φ(1)≈0.841
From tables: Φ(1)≈0.8413.
Empirical Rule (68-95-99.7)
For any normal N(μ,σ2):
Interval
Coverage
μ±σ
≈68%
μ±2σ
≈95%
μ±3σ
≈99.7%
This is useful for quick estimates.
Exact Values
Φ(1)−Φ(−1)=0.8413−0.1587=0.6826
Φ(2)−Φ(−2)=0.9772−0.0228=0.9544
Φ(3)−Φ(−3)=0.9987−0.0013=0.9974
Sum of Independent Normals
If X∼N(μ1,σ12) and Y∼N(μ2,σ22) are independent:
X+Y∼N(μ1+μ2,σ12+σ22)
The sum of independent normals is normal. This is not true for arbitrary sums.