Intuition
A quantity is conserved when nothing about it changes as the system evolves: not its average, not its spread, not the probability of any of its values. The test is a single commutator — an observable that commutes with the Hamiltonian is conserved, in every state. Energy always is. And the energy–time relation says how fast anything can change when the energy is spread by a given amount.
An ice skater spinning with no friction keeps her angular momentum however she moves her arms. In quantum mechanics the promise is stronger: the whole probability distribution of a conserved quantity stays exactly as it was.
Conservation laws
The rate of change of any expectation value is the average of the commutator of the Hamiltonian with the observable. If the commutator vanishes the average is constant in every state, and so is the probability of each eigenvalue: the observable is conserved.
What conservation means
- Energy is conserved for a time-independent , since .
How averages change
Differentiate the bracket with the product rule and use the Schrödinger equation for the ket and its adjoint for the bra. The two terms are the Hamiltonian acting before and after the observable, and together they make the commutator.
Proof steps
The product rule, for an observable that does not depend on time itself.
and its adjoint.
Collect the two terms into a commutator.
A vanishing commutator makes the average constant in every state.
Applications
Practice
The Commutator Test
The average of an observable changes at a rate given by the average of its commutator with the Hamiltonian. If that commutator is zero, the observable is conserved.
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For , which observable is conserved?
Energy Is Conserved
Every operator commutes with itself, so for a Hamiltonian that does not depend on time the energy is always conserved.
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For a time-independent Hamiltonian, the probability of each energy eigenvalue stays constant in time.
Conserved Means Shared Eigenstates
An observable that commutes with the Hamiltonian can be diagonalised together with it, so energy eigenstates can be chosen with definite values of it too.
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Why are energy levels often labelled by the eigenvalues of conserved observables?
Using the Rate Formula
For an observable that does not commute with , the rate of change of its average is times the average of the commutator.
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In some state . What is ?
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If , only the average of is conserved; its spread can still change.
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A state has an energy spread per nanosecond. What is the shortest time, in nanoseconds, in which any observable's average can change by one standard deviation?
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What does the energy–time relation say about a state with ?
Final checkpoint
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If , then changes in every state.
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An excited state lives about ns. Using and eV s, what is its energy spread, in units of eV? Give two decimal places.
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For a free particle, . Which quantity is conserved besides the energy?
Completion
Lesson complete
Great work! You now know how to:
- find the rate of change of an average from a commutator
- test an observable for conservation
- use the energy–time relation to link energy spread and speed of change