Conserved Quantities
Some quantities never change as a system evolves — energy, and often momentum, charge, or spin along an axis. Quantum mechanics gives a crisp, operator-level criterion for which observables are conserved.
The conservation criterion
Ehrenfest's theorem, for an observable with no explicit time dependence, reads
If commutes with the Hamiltonian, , then the right-hand side vanishes for every state, so
Such an is a constant of the motion. The statement is stronger than "the average is constant in one state" — commuting with makes the expectation value (and, as shown below, the full probability distribution of ) constant in all states.
Energy is always conserved (for time-independent H)
The Hamiltonian commutes with itself, , so is conserved whenever does not depend explicitly on time. Energy conservation is the most basic instance of the criterion, and it follows with no extra assumptions.
Conserved means more than a steady average
When , the two operators can be simultaneously diagonalised: there is a common eigenbasis labelled by both energy and the value of . Time evolution only multiplies each such basis state by a phase , which does not move probability between different -eigenvalues. So the entire probability distribution of the measurement of — not merely its mean — is frozen in time.
A simple check
For a spin with , the observable commutes with (they are the same operator up to a constant), so is conserved — consistent with the previous lesson's staying flat. By contrast does not commute with (), so is free to oscillate — and it does, as .
Try it
This is a numerical exercise — your code should return a number. Verify that is
conserved under by computing the relevant commutator entry of
, which must be (hence ).
Sign in on the full site to ask questions and join the discussion.