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Boundary conditions, quantization, and expansion in eigenstates
The infinite square well is the simplest quantum system that exhibits energy quantization. This module solves the time-independent Schrodinger equation inside the well, applies boundary conditions, finds the energy spectrum and eigenfunctions, and shows how arbitrary initial states evolve by expansion in the energy eigenbasis.
Consider a particle confined to a region where the potential is zero, with infinite walls at and :
Outside the well, the wave function must be zero because the particle cannot exist where . Inside the well (), the time-independent Schrödinger equation becomes:
The general solution is , where . The boundary condition gives . The boundary condition requires , so for integer
The quantum number is excluded because it would give everywhere, which is not normalizable. Negative values of give the same physical states as positive (up to an overall sign), so we restrict to .
Potential
Inside the well
Quantized wave numbers
Energy eigenvalues
Normalized eigenfunctions
The energy levels are quantized: where is the ground state energy. The spacing between adjacent levels increases with : .
The eigenfunctions are orthonormal: . This can be verified using trigonometric identities.
The eigenfunctions form a complete set: any reasonably well-behaved function on can be expanded as a Fourier sine series: . This is precisely the expansion we need to solve the time-dependent problem.
The th eigenfunction has nodes (zeros) inside the well. The ground state () has no nodes, the first excited state () has one node at , and so on. More nodes correspond to higher energy, a general feature of quantum mechanics.
Ground state energy
Orthonormality
Completeness
Number of nodes
The infinite square well: a particle confined between impenetrable walls at x = 0 and x = a. The wave function ψ_n (blue) must have nodes at the walls. The probability density |ψ_n|² (purple) shows where the particle is likely to be found. Energy levels E_n ∝ n² are quantized. Toggle "Classical" to see the uniform probability expected from classical physics.
Given an initial wave function , we expand it in the energy eigenbasis:
The expansion coefficients are found by Fourier's trick: multiply both sides by and integrate, using orthonormality:
The full time-dependent solution attaches the phase factor to each term:
Although each stationary state has a time-independent probability density, a superposition does not. The probability density can exhibit complex time-dependent behavior, including oscillations and revivals.
Initial expansion
Expansion coefficients
Time-dependent solution
A particle in an infinite square well of width has initial wave function . Find the expansion coefficients, the probability of the ground state, and the expectation value of the energy.
Step 1 — Normalization. . Thus .
Step 2 — Expansion coefficients. . Using integration by parts twice, . Only odd contribute.
Step 3 — Ground state probability. . The particle is almost certainly in the ground state because the parabolic initial state closely resembles .
Step 4 — Energy expectation value. .
Initial state
Expansion coefficients
Ground state probability
Energy expectation
Papers:
David J. Griffiths, Introduction to Quantum Mechanics, 2nd ed., Chapter 2: Time-Independent Schrodinger Equation (Section 2.2)
1. What are the energy levels of the infinite square well?
2. Why is excluded?
3. How many nodes does the th eigenfunction have?
4. What determines the quantization of energy?
5. Are the eigenfunctions of the infinite square well complete?