Checkpoint: Stationary States
A stationary state is a solution of the Schrödinger equation that has a single, definite energy. They arise when the potential does not depend on time, so that the Schrödinger equation separates: write and substitute into
Dividing both sides by yields a left side that depends only on and a right side that depends only on . Both must equal the same constant , giving two ordinary differential equations. The time equation is solved immediately:
This oscillatory factor carries no physical probability weight on its own — — which is why a stationary state has a time-independent probability density:
The spatial part satisfies the time-independent Schrödinger equation (TISE):
The infinite square well
The simplest non-trivial potential traps a particle inside a box of width with infinitely hard walls: for and elsewhere. The infinite walls force . Inside the box the TISE reduces to
The general solution is . The boundary condition forces . The condition then requires for a positive integer , giving the quantization condition
Substituting back yields the discrete energy levels:
where the ground-state energy is
The key result is that energies grow as : the second level is four times the ground state, the third level is nine times, and so on. This scaling is a fingerprint of the infinite square well.
The normalized wave functions
Normalizing over gives , so
Each has nodes (zeros strictly inside the well) — has no internal nodes, has one, and so on.
Phase evolution of a stationary state
Each stationary state acquires a phase at a rate :
Multiplying by a pure phase factor does not change any probability. That is the precise sense in which these are "stationary" states — the physics (all expectation values, all probabilities) is frozen in time, even though the complex amplitude rotates.
When two stationary states are superposed, the two phase factors rotate at different rates and , and their interference pattern oscillates at the beat frequency . This is how the time-dependence reappears in non-stationary states.
Numerical scale: an electron in a 1 nm box
For an electron () in a well of width ,
The third level therefore sits at — a few electron-volts, the same scale as electronic energies in atoms and molecules. What spectroscopy actually measures is the difference between levels: here , a photon of wavelength at the violet edge of the visible range. Nanometre-scale confinement is what puts these gaps into the optical band, the effect exploited in quantum-dot spectroscopy.
Try it
This is a numerical exercise — return a number. Compute the energy of the stationary
state of an infinite square well of width , for an electron, in eV.
Build it from first principles: calculate from the formula above, then multiply by .
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