- 4,796
- 32
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 and implications of the time-energy uncertainty relation, specifically the expression \(\Delta E \Delta t \geq \hbar/2\). Participants explore its applicability, the meaning of \(\Delta t\), and the differences between this relation and other uncertainty principles, such as position-momentum.
Participants express differing interpretations of the time-energy uncertainty relation, with no consensus on a single definition or application. Some agree on certain mathematical interpretations, while others challenge the existence of a time operator and the nature of \(\Delta t\).
Discussions include various interpretations and definitions of \(\Delta t\), with some participants emphasizing the need for careful interpretation and noting that the relation may not be universally applicable in the same way as other uncertainty principles.
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}