Correspondence Principle
Also known as: Bohr's correspondence principle · Classical limit
Quantum mechanics can't just contradict the classical physics we see every day — it must reproduce it in the right limit. Bohr's principle says: for large quantum numbers (highly excited states) or when actions are huge compared to ℏ, quantum predictions blur into classical ones. A hydrogen electron in orbit n=1000 radiates almost exactly like a classical charge going around a loop. It's the guardrail that kept early quantum theory tethered to known physics.
As n grows, the discrete quantum energy levels crowd together and the ladder blurs into the classical continuum.
Equivalent forms
Every good quantum theory must contain the old classical one hiding inside its large-n or ℏ→0 corner — a consistency demand, not an accident.
Where it holds
Dimensional analysis
Bohr articulated the principle around 1913–1920 while building his atomic model: the frequency of light emitted between high-n orbits matches the electron's classical orbital frequency. He used it as a bridge to guess quantum selection rules before a full theory existed, and named it explicitly in 1920.
- Justifying classical mechanics for macroscopic bodies
- Semiclassical (WKB) methods and quantum-classical modeling
- Rydberg-atom and quantum-chaos studies
- The classical limit is large action (S≫ or large n, not literally in nature
- Quantum→classical is not automatic for all states — Schrödinger-cat and entangled states resist it
- It's a consistency guide, not a derivation of classical mechanics
What if…
Levels are far apart relative to their energy — the system is deeply quantum and shows no classical resemblance.
The Schrödinger equation reduces (via WKB) to the classical Hamilton–Jacobi equation — classical trajectories reappear.
Vanishing relative spacing
- |,
- (very quantum); (nearly continuous)