Solving the Schrödinger equation for the harmonic oscillator Hamiltonian reveals a remarkable result: only a discrete set of energy values leads to physically acceptable (normalizable) wavefunctions. These allowed energies are the vibrational energy levels of the system.
Normalizable wavefunctions and allowed energies
The time-independent Schrödinger equation for the harmonic oscillator,
\[ \hat{H}\psi(x) = \left( -\frac{\hbar^2}{2\mu}\frac{d^2}{dx^2} + \frac{1}{2}kx^2 \right)\psi(x) = E\psi(x), \]
admits solutions for many mathematical values of \(E\). However, most of these solutions are not physically acceptable: they diverge as \(|x|\rightarrow\infty\) and cannot be normalized.
Requiring the wavefunction to remain finite and normalizable restricts the allowed energies to a discrete set. Only for these special values of \(E\) do the solutions decay to zero at large displacements.
Quantized vibrational energy levels
The allowed energy levels of the quantum harmonic oscillator are
\[ E_v = \hbar\omega\left(v + \frac{1}{2}\right), \qquad v = 0, 1, 2, \ldots \]
where \(v\) is the vibrational quantum number and \( \omega = \sqrt{k/\mu} \) is the angular vibrational frequency.
The appearance of discrete energy levels is a direct consequence of the boundary conditions imposed by normalizability, not by any explicit restriction placed on the energy in advance.
Zero-point energy
Even in the lowest vibrational state (\(v=0\)), the energy is not zero:
\[ E_0 = \frac{1}{2}\hbar\omega. \]
This zero-point energy reflects the fact that a quantum particle cannot be completely at rest. The simultaneous requirements of confinement and the uncertainty principle prevent both the position and momentum from being exactly zero.
Big idea: the vibrational energy levels of the harmonic oscillator arise because only certain energies produce wavefunctions that remain finite and normalizable. Quantization is therefore a consequence of the mathematical and physical requirements placed on the solutions of the Schrödinger equation.