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How should \Delta E \Delta t \geq \hbar/2 be interpreted? When does it apply? Delta t refers to the time of what? etc.
Thx.
Thx.
The discussion centers on the interpretation of the time-energy uncertainty relation, expressed as ΔE Δt ≥ ℏ/2. Participants clarify that Δt represents the characteristic time for an observable to change by one standard deviation, defined as Δt := ΔA / |d⟨A⟩/dt|. The conversation emphasizes that this relation does not imply a time operator exists, but rather describes the evolution of a system's energy over time. The participants reference Heisenberg's inequality and the importance of understanding the physical meaning behind the relation, highlighting that Δt is a duration of a physical process rather than an uncertainty in time.
PREREQUISITESQuantum physicists, students of quantum mechanics, and researchers interested in the foundations of quantum theory will benefit from this discussion. It provides insights into the interpretation of the time-energy uncertainty relation and its implications for quantum state evolution.
To be precise there is no such thing as a time-energy uncertainty principle. Uncertainty principles are the relationship between two operators and while there is an energy operator there is no such thing as a time operator. Best to call it the time-energy uncertainty relation. The meaning of this relation is dt is the amount of time it takes for a system to evolve and dE represents the average change in the amount of energy during this time of evolution.quasar987 said:How should \Delta E \Delta t \geq \hbar/2 be interpreted? When does it apply? Delta t refers to the time of what? etc.
Thx.
Galileo said:And using:
\frac{d\langle A\rangle}{dt}=\frac{i}{\hbar}\langle [H,A]\rangle
In this approach, Delta t is NOT UNCERTAINTY of time, but a time DURATION of a physical process. There is however a similar way to introduce UNCERTAINTY of time measured by a clock, as explained, e.g., inGalileo said:For a given time independent observable A that doesn't commute with the Hamiltonian and a state |psi>, interpret \Delta E = \Delta H (H is the hamiltonian and delta means standard deviation) and define:
\Delta t := \frac{\Delta A}{|d\langle A \rangle/dt|}
So \Delta t is the characteristic time it takes for the observable to change by one standard deviation.
I think this is the best interpretation of the inequality. No mystic mojo is involved.
Then by Heisenberg's inequality:
\Delta H \Delta A \geq \frac{1}{2}|\langle [H,A] \rangle|
And using:
\frac{d\langle A\rangle}{dt}=\frac{i}{\hbar}\langle [H,A]\rangle
you can rewrite it as \Delta E \Delta t \geq \frac{\hbar}{2}