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🧤Physical Chemistry I Unit 15 Review

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15.3 Wave functions and probability distributions

15.3 Wave functions and probability distributions

Written by the Fiveable Content Team • Last updated August 2025
Written by the Fiveable Content Team • Last updated August 2025
🧤Physical Chemistry I
Unit & Topic Study Guides

Wave function interpretation

Physical meaning and Born interpretation

A wave function, written as Ψ(x,t)\Psi(x, t), is a complex-valued function that fully describes the quantum state of a particle as a function of position and time. On its own, the wave function doesn't correspond to anything you can directly measure. What gives it physical meaning is the Born interpretation.

The Born interpretation states that Ψ(x,t)2|\Psi(x, t)|^2 gives the probability density for finding the particle at position xx at time tt. More precisely, Ψ(x,t)2dx|\Psi(x,t)|^2 \, dx is the probability of finding the particle in an infinitesimal interval dxdx around xx. This is what bridges the abstract math of wave functions to measurable outcomes.

In the double-slit experiment, for instance, the wave function passes through both slits simultaneously and interferes with itself. The resulting Ψ2|\Psi|^2 on the detection screen produces the characteristic interference pattern, with alternating bands of high and low probability.

Probability density and its relation to the wave function

Because Ψ\Psi is generally complex-valued, you obtain the probability density by multiplying the wave function by its complex conjugate:

Ψ(x,t)2=Ψ(x,t)Ψ(x,t)|\Psi(x,t)|^2 = \Psi^*(x,t)\,\Psi(x,t)

This guarantees a real, non-negative result, which is necessary for something representing a probability.

The wave function itself can be positive, negative, or complex, and those signs/phases matter for interference effects. But only the squared modulus has a direct physical interpretation as probability density.

For a particle in a one-dimensional box (ground state), the probability density is highest at the center of the box and goes to zero at the walls. For higher energy states, the probability density develops nodes (points where it equals zero) between the walls.

Probability density and distribution

Physical meaning and Born interpretation, 27.3 Young’s Double Slit Experiment – College Physics

Calculating probability density

To find the probability that a particle is located within a specific region [a,b][a, b], you integrate the probability density over that region:

P(axb)=abΨ(x,t)2dxP(a \leq x \leq b) = \int_a^b |\Psi(x,t)|^2 \, dx

Step-by-step process:

  1. Start with the wave function Ψ(x,t)\Psi(x, t) for the system.
  2. Compute the probability density: Ψ(x,t)2=ΨΨ|\Psi(x,t)|^2 = \Psi^* \Psi.
  3. Integrate Ψ2|\Psi|^2 from aa to bb to get the probability of finding the particle in that interval.

For example, to find the probability of locating an electron in the left half of a one-dimensional box of length LL, you'd integrate Ψ(x)2|\Psi(x)|^2 from 00 to L/2L/2.

Probability distribution and its properties

The probability distribution across all space must satisfy two key properties:

  • Non-negativity: Ψ(x,t)20|\Psi(x,t)|^2 \geq 0 everywhere, since probabilities can't be negative.
  • Normalization: The total probability of finding the particle somewhere must equal one:

Ψ(x,t)2dx=1\int_{-\infty}^{\infty} |\Psi(x,t)|^2 \, dx = 1

Different potentials produce different probability distributions. For a quantum harmonic oscillator in its ground state, the probability distribution is a Gaussian centered at the equilibrium position. The width of that Gaussian depends on the oscillator frequency ω\omega and the particle mass mm, specifically through the characteristic length scale /(mω)\sqrt{\hbar / (m\omega)}.

Normalization of wave functions

Physical meaning and Born interpretation, Young’s Double-Slit Interference – University Physics Volume 3

Purpose of normalization

Normalization ensures that the total probability of finding the particle somewhere in all of space equals exactly one. Without this, the Born interpretation breaks down because the probabilities extracted from Ψ2|\Psi|^2 wouldn't be meaningful.

Any valid solution to the Schrödinger equation can be multiplied by a constant and still be a solution. Normalization pins down that constant so the probabilistic interpretation holds. For example, in a two-state system like a spin-1/2 particle, normalization guarantees that the probabilities of measuring spin-up and spin-down sum to one.

Procedure for normalizing wave functions

  1. Start with an unnormalized wave function Ψ(x)\Psi(x) (possibly containing an unknown constant AA).
  2. Compute the integral Ψ(x)2dx\int_{-\infty}^{\infty} |\Psi(x)|^2 \, dx.
  3. Set that integral equal to 1 and solve for the normalization constant AA.
  4. Multiply the original wave function by AA to get the normalized version.

Worked example: For a Gaussian wave function Ψ(x)=Aex2/(2σ2)\Psi(x) = A\,e^{-x^2/(2\sigma^2)}:

  • Compute A2ex2/σ2dx=A2πσ\int_{-\infty}^{\infty} |A|^2 e^{-x^2/\sigma^2} dx = |A|^2 \sqrt{\pi}\,\sigma
  • Set equal to 1: A2πσ=1|A|^2 \sqrt{\pi}\,\sigma = 1
  • Solve: A=(1π1/2σ)1/2A = \left(\frac{1}{\pi^{1/2}\,\sigma}\right)^{1/2}

This value of AA ensures Ψ(x)2dx=1\int_{-\infty}^{\infty} |\Psi(x)|^2 dx = 1.

Expectation values from wave functions

Definition and calculation of expectation values

The expectation value of an observable is the average result you'd obtain if you measured that observable on a large number of identically prepared systems. It's not necessarily a value you'd get in any single measurement.

For an observable with corresponding operator O^\hat{O}, the expectation value is:

O=Ψ(x)O^Ψ(x)dx\langle O \rangle = \int_{-\infty}^{\infty} \Psi^*(x)\,\hat{O}\,\Psi(x)\, dx

Note the order: the complex conjugate Ψ\Psi^* goes on the left, the operator acts on Ψ\Psi on the right, and you integrate over all space.

For energy, the relevant operator is the Hamiltonian:

H^=22md2dx2+V(x)\hat{H} = -\frac{\hbar^2}{2m}\frac{d^2}{dx^2} + V(x)

So the expectation value of energy is E=ΨH^Ψdx\langle E \rangle = \int_{-\infty}^{\infty} \Psi^* \hat{H}\,\Psi \, dx.

Expectation values of position and momentum

Position: The position operator is simply x^=x\hat{x} = x, so:

x=Ψ(x)xΨ(x)dx\langle x \rangle = \int_{-\infty}^{\infty} \Psi^*(x)\, x \,\Psi(x)\, dx

Momentum: The momentum operator in the position representation is p^=iddx\hat{p} = -i\hbar\frac{d}{dx}, so:

p=Ψ(x)(iddx)Ψ(x)dx\langle p \rangle = \int_{-\infty}^{\infty} \Psi^*(x)\left(-i\hbar\frac{d}{dx}\right)\Psi(x)\, dx

Here \hbar is the reduced Planck constant (h/2πh/2\pi).

These expectation values connect quantum theory to experiment. For a quantum harmonic oscillator in any energy eigenstate, both x=0\langle x \rangle = 0 and p=0\langle p \rangle = 0 due to the symmetry of the potential about the equilibrium position. This doesn't mean the particle is stationary; it means the average position and average momentum are zero because the particle spends equal time on either side and moving in either direction.

To characterize the spread of a particle's position or momentum, you also need x2\langle x^2 \rangle and p2\langle p^2 \rangle. The standard deviations Δx=x2x2\Delta x = \sqrt{\langle x^2 \rangle - \langle x \rangle^2} and Δp=p2p2\Delta p = \sqrt{\langle p^2 \rangle - \langle p \rangle^2} are what appear in the Heisenberg uncertainty principle: ΔxΔp/2\Delta x \, \Delta p \geq \hbar/2.

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