FKM Kompass
L3

The Schrödinger equation

The Schrödinger equation is the central equation of non-relativistic quantum mechanics, playing the same role for a wavefunction that Newton's second law plays for a classical trajectory — given the forces acting on a particle, it determines exactly how the wavefunction evolves in time.

Practise this concept

Classical mechanics has one central equation of motion, F = ma, that turns a description of the forces acting on an object into a prediction of exactly how its position changes over time. Quantum mechanics has an analogous central equation, but for the wavefunction rather than a trajectory: the Schrödinger equation, which takes the potential energy a particle experiences and determines exactly how its wavefunction evolves in time. The two equations play parallel structural roles — each is the engine that turns "here are the forces" into "here is how the state changes" — but what they each act on is fundamentally different: a definite position and velocity in one case, a probability-carrying wavefunction in the other.

Solving the equation for a particular physical situation — a particle confined to a box, an electron bound to a proton, a mass on a spring — typically does not yield one wavefunction with one energy, but a whole family of solutions, each pairing an allowed wavefunction with its own energy value. This is not the equation malfunctioning; it is exactly how quantisation emerges within this framework. The particle-in-a-box's discrete energy ladder and the hydrogen atom's discrete spectral lines are both directly consequences of the Schrödinger equation admitting only certain wavefunctions for a given confining potential, precisely the same way a guitar string clamped at both ends admits only certain standing-wave patterns.

Time-independent versions of the equation, used for situations where the system's energy does not change, are what produce these discrete energy levels directly; the full time-dependent equation is needed whenever the wavefunction itself changes shape over time — a wave packet spreading, interfering, or tunnelling through a barrier. Both versions apply to any non-relativistic quantum system once its potential energy is specified, not merely to hydrogen or any other single example; the equation is general, and each different physical situation is simply a different choice of potential fed into the same governing structure.

Key ideas

Requires: Wavefunctions and probability

Unlocks: Basics of molecular quantum mechanics, Operators and observables, Potential steps and finite wells, The Heisenberg picture and time-dependent perturbation theory, Quantum numbers and atomic orbitals, The quantum harmonic oscillator

Common misconceptions

  • The Schrödinger equation predicts a particle's exact position at each moment, just as Newton's laws do.
  • Solving the Schrödinger equation always gives a unique, unambiguous energy for a system.
  • The Schrödinger equation only applies to hydrogen-like atoms, not to other quantum systems.

Resources

Part of these UT courses

This concept is mapped as covering part of the following course(s) in the University of Tartu curriculum.