Physic Labs

Quantum mechanics

The quantum harmonic oscillator

Observe the stationary states of the quantum oscillator: probability density and energy-level position as a function of quantum number n. Verify the evenly spaced spectrum En=ℏω(n+12)E_n = \hbar\omega\left(n + \tfrac{1}{2}\right) and the nonzero zero-point energy.

Undergraduate

Equipment

  • 3D canvas plotting probability density and energy levels, rotated by dragging or arrow keys
  • Slider «Số lượng tử n» selecting the eigenstate from n = 0 to n = 5
  • Readout line showing «Eₙ/ℏω» and the spacing «Eₙ₊₁ − Eₙ = ℏω»

Procedure

  1. Observe the ground state n = 0

    Set «Số lượng tử n» = 0: the canvas shows a bell-shaped probability density with no node, and the readout reports «Eₙ/ℏω = 0.5». Note the zero-point energy E0=12ℏω≠0E_0 = \tfrac{1}{2}\hbar\omega \neq 0 — the particle cannot rest in the parabolic well.

  2. Sweep the excited levels and check the even spacing

    Step «Số lượng tử n» through 0 → 1 → 2 → 3 → 4 → 5. Each time record «Eₙ/ℏω» and check that consecutive levels differ by «Eₙ₊₁ − Eₙ = ℏω». Compare with En=ℏω(n+12)E_n = \hbar\omega\left(n + \tfrac{1}{2}\right): the readings must be 0.5, 1.5, 2.5, 3.5, 4.5, 5.5 in turn.

  3. Count nodes and study the probability density shape

    At each level n, drag the canvas to rotate the view and count the nodes (zero-density points) of the probability density: exactly n of them, with tails leaking into the classically forbidden region. Observe that for large n the density concentrates near the two turning points, approaching the classical distribution.

  4. Compare with the classical oscillator and predict

    Before moving «Số lượng tử n» to a new value, predict «Eₙ/ℏω» using En=ℏω(n+12)E_n = \hbar\omega\left(n + \tfrac{1}{2}\right) and check the readout. Conclude: unlike the classical oscillator that accepts any continuous energy, the quantum oscillator admits only evenly spaced levels with lowest energy ℏω/2\hbar\omega/2.

Simulation

Experiment history

Max Planck introduced quantised energy for the blackbody problem in 1900, treating oscillators that exchange energy in multiples of hν. In modern quantum mechanics, Erwin Schrödinger in 1926 solved the wave equation for the parabolic potential and obtained evenly spaced levels En=ℏω(n+1/2)E_n = \hbar\omega(n+1/2) with Hermite–Gauss eigenfunctions; Werner Heisenberg had derived the same spectrum from matrix mechanics in 1925. Also in 1926 Paul Dirac developed the creation–annihilation operator method a† and a, turning the whole problem into counting the level index n — a foundational tool of quantum field theory and quantum optics. The zero-point energy ℏω/2\hbar\omega/2 is a direct consequence of the uncertainty principle: a particle confined in a parabolic potential cannot be at rest.

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