A wavefunction ψ(x) is only physically meaningful if the total probability of finding the
particle somewhere equals exactly one:
∫−∞∞∣ψ(x)∣2dx=1.
This requirement is called normalization. It follows directly from the Born rule: if
∣ψ(x)∣2 gives the probability density, the entire probability density must integrate to one
over all space.
The normalization constant
In practice, we often start with an unnormalized function ψ~(x) and write
ψ(x)=Aψ~(x),
where A is a real positive constant chosen so that ψ is normalized. Substituting:
∫∣ψ(x)∣2dx=A2∫∣ψ~(x)∣2dx=1⟹A=∫∣ψ~(x)∣2dx1.
All that remains is to compute the integral of ∣ψ~∣2 and take the reciprocal square root.
A worked example
Consider the trial wavefunction defined on the interval [0,L]:
Setting L=1 gives the integral 301, so the normalization constant is
A=1/301=30.
Substituting back confirms ψ(x)=30x(1−x) is normalized:
30∫01x2(1−x)2dx=30⋅301=1.✓
Try it
This is a numerical exercise — your code should return a number. Given ψ(x)=A⋅x(1−x)
on [0,1] and zero elsewhere, compute the positive normalization constant A.
Run your code to see the quantum state.
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