The Born rule says that a particle with (normalised) wavefunction ψ(x) is found in the
interval [a,b] with probability
P(a≤x≤b)=∫ab∣ψ(x)∣2dx.
The integrand ∣ψ(x)∣2 is the probability density — it is always real and non-negative,
and it integrates to 1 over all space by the normalisation condition.
A worked example: the infinite square well
Consider a particle confined to a one-dimensional box of width L. Inside the box the walls are
infinitely high, so the wavefunction must vanish at both walls. The ground state (lowest energy,
n=1) satisfying this boundary condition and the normalisation condition is
ψ1(x)=L2sin(Lπx),0≤x≤L,
and ψ1(x)=0 everywhere outside the box. You can confirm normalisation directly:
∫0L∣ψ1∣2dx=L2∫0Lsin2(Lπx)dx.
Using sin2θ=21(1−cos2θ) the integral becomes
L2⋅2L=1. Good.
Finding the probability in an interval
Take L=1m for simplicity. The probability of finding the particle in the left third
of the box, 0≤x≤31, is
P=∫01/32sin2(πx)dx.
Apply the identity sin2θ=21−cos2θ:
P=∫01/3(1−cos(2πx))dx=[x−2πsin(2πx)]01/3.
Evaluating the boundary terms and using sin(2π/3)=3/2:
P=31−2πsin(2π/3)=31−2π3/2=31−4π3≈0.1955.
Why this matters
Every measurable quantity in quantum mechanics ultimately reduces to an integral of this form —
or a sum of such integrals for discrete spectra. Mastering the mechanics of evaluating ∫∣ψ∣2dx
over a chosen region is therefore a foundational skill for all subsequent quantum calculations.
Try it
This is a numerical exercise — return a number. The ground state of an infinite square well of
width L=1m has wavefunction ψ(x)=2sin(πx) for 0≤x≤1.
Compute the probability of finding the particle in the left third of the well
(0≤x≤31).
Run your code to see the quantum state.
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