Context:FIT2086_MOC · the default parametric model for X=R · two parameters θ=(μ,σ2) that are the mean and variance · self-similar and additive, which is why it carries the confidence-interval and regression work later in the unit
Quick Revision
🎯 Objective:X∼N(μ,σ2) with
p(x∣μ,σ2)=(2πσ21)1/2exp(−2σ2(x−μ)2)
➔ symmetric bell on all of R, tailing to 0 as ∣x∣→∞.
⚡ Key Constraint: the cdf has no closed form — every probability comes from standardising to Z and reading a table, or from pnorm in R. Never try to integrate the pdf by hand.
📝 How It Works
1. The density and its parameters
Parameters are the moments ➔ θ=(μ,σ2)∈Θ=R×R+, where μis the mean and σ2is the variance — unusually direct; most distributions require deriving E[X]=f(θ).
Shape ➔ symmetric about μ; σ2 controls width (small σ2 ⟹ tall narrow peak, large σ2 ⟹ low flat spread).
Centrality collapse ➔ symmetry ⟹ mode = median = mean =μ (contrast the skewed cases in Measures of Centrality).
Notation ➔ X∼N(μ,σ2), "∼" read as “is distributed as per a”.
2. Self-similarity (standardisation)
Every Gaussian is a rescaled standard normal ➔ if Z∼N(0,1) then X=σZ+μ is N(μ,σ2).
Inverted, this is the z-score ➔ Z=σX−μ ➔ one table/one function serves all(μ,σ2).
Consistency check ➔ E[σZ+μ]=σ⋅0+μ=μ and V[σZ+μ]=σ2V[Z]=σ2 by [[Expectations and Covariance (FIT2086)|linearity and V[cX]=c2V[X]]].
Why the σ-rules are scale-free ➔ standardising a bound of the form μ+kσ gives Zμ+kσ=σ(μ+kσ)−μ=k ➔ the z-score does not depend on μ or σ at all, so ∫μ−σμ+σp(x∣μ,σ2)dx=∫−11p(x∣0,1)dx≈0.6825 for every parameter pair.
Reading a z-score ➔ it is a standardised distance from the mean, in standard-deviation units — which is why one table answers every question.
3. The cdf and the σ-rules
No closed form ➔ evaluated numerically by software; the reason z-tables exist at all.
Scale-free coverage rules (hold for everyμ,σ):
Interval
Probability mass
(μ−σ,μ+σ)
68.27%
(μ−2σ,μ+2σ)
95.45%
(μ−3σ,μ+3σ)
99.73%
Why they are useful ➔ they convert a distance-from-the-mean into a probability with no integration, and are the intuition behind later confidence intervals.
4. Additivity and decomposition
Sum of two independent Gaussians is Gaussian ➔ X1∼N(μ1,σ12), X2∼N(μ2,σ22) ⟹
X1+X2∼N(μ1+μ2,σ12+σ22)
— means add, variances add (never standard deviations).
Decomposition (the converse) ➔ for any n≥1, X∼N(μ,σ2) can be written X=∑i=1nXi with Xi∼N(μi,σi2) whenever ∑μi=μ and ∑σi2=σ2 ➔ a normal RV splits into arbitrarily many normal pieces.
📊 Exam Execution Trace & Applied Exercises
Manual Execution Trace — standardise, then read the cdf
X∼N(100,152); find P(X≤118) and P(85<X<115).
Step
Operation
Computation
Result
1
standardise the bound
z=15118−100
z=1.2
2
cdf lookup / pnorm
P(Z≤1.2)
≈0.885
3
recognise 85,115 as μ±σ
σ-rule
68.27%
4
upper tail
1−P(X≤118)
≈0.115
Key move: step 3 needs no table at all — spotting that the interval isμ±kσ collapses the question to a memorised rule.
Manual Execution Trace — reading a coarse z-table by interpolation (Studio 2)
The provided table is indexed by ∣z∣ with two probability columns — P(Z<−∣z∣) (lower tail) and P(Z<∣z∣) (upper) — at a coarse step of 0.093, so an exam z almost never appears in it. Linear interpolation between the bracketing rows is the intended hand skill:
P(Z<z)≈Plo+zhi−zloz−zlo(Phi−Plo)X∼N(3,16), i.e. μ=3, σ=16=4:
Target
Standardise
Column + bracketing rows
Interpolate
Answer
P(X<5)
z=45−3=0.5
P(Z<∣z∣): 0.465→0.679076, 0.558→0.711625
0.679076+0.0930.035(0.032549)=0.6913
≈0.69
P(X>−4)
z=4−4−3=−1.75
P(Z<−∣z∣) at ∣z∣=1.75: 1.674→0.047024, 1.767→0.038577
Key moves: (i) N(3,16) carries the variance ➔ divide by σ=4, never by 16; (ii) the table is indexed by ∣z∣, so a negativez means looking up ∣z∣ in the P(Z<−∣z∣) column — the sign selects the column, not a subtraction; (iii) an interval probability is F(zhi)−F(zlo), one interpolated lookup each.
Applied Exercise — additivity
Problem:X1∼N(3,4) and X2∼N(5,9) are independent. Distribution of X1+X2, and P(X1+X2>12)?
dnorm(x, mean = 0, sd = 1) # density height at x — NOT a probabilitypnorm(118, mean = 100, sd = 15) # cdf P(X <= 118) = 0.8849pnorm(118, 100, 15, lower.tail = FALSE) # upper tail P(X > 118)qnorm(0.975) # quantile: 1.96rnorm(n, mean = 100, sd = 15) # n random draws# Studio 2 — the sigma-rule and the z-score equivalencepnorm(1, 0, 1) - pnorm(-1, 0, 1) # 0.6825 — and identical for ANY (mu, sigma):pnorm(7, 2, 5) - pnorm(-3, 2, 5) # mu +/- sigma = 2 +/- 5pnorm(12,10,2) - pnorm(8, 10, 2) # mu +/- sigma = 10 +/- 21 - pnorm(2, 0, 1) # P(X > 2), X ~ N(0,1) = 0.02271 - pnorm(2, 0, 4) # P(X > 2), X ~ N(0,4^2) = 0.30851 - pnorm((2 - 0)/4, 0, 1) # SAME — standardise, then use N(0,1)
💡 Common Mistake: R takes sd, not the variance ➔ for N(100,152) pass sd = 15; passing 225 silently models N(100,2252). The last two lines above are the computational face of self-similarity: standardising by hand and calling pnorm on N(0,1) is the same calculation as passing (μ,σ) directly.
⚠️ Common Mistakes
💡 σ2 vs σ ➔ the notation N(μ,σ2) carries the variance, but standardising and R’s sd argument both need σ. Mis-rooting is the single largest mark-loss vector here.
💡 Adding standard deviations ➔ under independence, variances add: σ=σ12+σ22, never σ1+σ2.
💡 Trying to integrate the pdf ➔ there is no closed-form antiderivative; standardise and use a table or pnorm.
💡 ≤ vs < ➔ irrelevant here (X is continuous, so P(X=x)=0) but the same slip is fatal for the discrete distributions.
💡 Reading a coarse z-table without interpolating ➔ snapping z=0.5 to the tabulated 0.465 costs accuracy the marker expects; interpolate between the bracketing rows.
💡 Double-complementing a negative z ➔ the table’s P(Z<−∣z∣) column already is the lower tail; P(X>−4)=1−P(Z<−1.75) needs exactly one subtraction.
🧠 Active Recall
What is self-similarity for the Gaussian, and why does it matter practically?
Answer
Short answer: every Gaussian is a translated and scaled standard normal — if Z∼N(0,1) then X=σZ+μ∼N(μ,σ2), equivalently Z=(X−μ)/σ.
Why:One tabulated distribution serves all parameters ➔ since the cdf has no closed form, every probability must be evaluated numerically; self-similarity means only N(0,1) need ever be tabulated, and any P(X≤x) becomes P(Z≤σx−μ). The moments follow by linearity: E[σZ+μ]=μ, V[σZ+μ]=σ2.
State the additivity property and give the parameters of X1+X2 for independent Gaussians.
Answer
Short answer:X1∼N(μ1,σ12), X2∼N(μ2,σ22) ⟹ X1+X2∼N(μ1+μ2,σ12+σ22) — the family is closed under addition, and conversely any N(μ,σ2) decomposes into n normal summands with ∑μi=μ, ∑σi2=σ2.
Why:Means add by linearity, variances add by independence ➔ E[X1+X2]=E[X1]+E[X2] holds unconditionally, while V[X1+X2]=V[X1]+V[X2] requires X1⊥X2; closure of the family is the extra Gaussian-specific fact.
Why is the mode of a Gaussian equal to its median and mean, and what fraction of mass lies within μ±2σ?
Answer
Short answer: the density is symmetric about μ with a single maximum there, so mode = median = mean =μ; 95.45% of the mass lies in (μ−2σ,μ+2σ).
Why:Symmetry forces the three location measures to coincide ➔ p(μ+d)=p(μ−d) makes μ both the balance point (mean) and the 0.5-quantile (median), and exp(−(x−μ)2/2σ2) is maximised where the exponent is zero, i.e. at x=μ (mode). The 68.27/95.45/99.73 coverage rules are scale-free, holding for every μ and σ.