Heisenberg principle, about time

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Discussion Overview

The discussion revolves around the Heisenberg uncertainty principle, specifically focusing on the relationship between energy and time. Participants explore the implications of measuring energy with high precision and the resulting uncertainty in the time at which that energy was present. The conversation touches on theoretical interpretations, measurement challenges, and conceptual clarifications related to quantum mechanics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant suggests that measuring energy with high precision leads to significant uncertainty in the corresponding time, questioning whether this time can extend into the future.
  • Another participant explains that if the energy is precisely known (ΔE=0), then the time uncertainty (Δt) becomes infinite, indicating a stationary state.
  • Some participants express confusion about the meaning of Δt, debating whether it represents a time interval or the time needed for a system to change states.
  • There is a discussion about the practical challenges of measuring energy, with suggestions that energy is often inferred from momentum measurements or transitions rather than directly measured.
  • A later contribution references a book that supports the idea that precise energy measurements do not provide information about the timing of emissions, reinforcing the notion that future times can be excluded.
  • Several participants note that the time-energy uncertainty relation is not a true uncertainty relation, as time is not treated as an operator in the same way as position or momentum.
  • Some participants propose analogies to help conceptualize the relationship between energy fluctuations and time intervals, though not all find these helpful.

Areas of Agreement / Disagreement

Participants express varying interpretations of the implications of the uncertainty principle, with no consensus on the exact nature of Δt or its relationship to future measurements. Some agree on the exclusion of future times in certain contexts, while others remain uncertain about the implications of the principle.

Contextual Notes

Participants highlight limitations in their understanding of quantum mechanics and the lack of emphasis on experimental methods in education. There are also references to specific conditions under which the uncertainty relations apply, indicating that the discussion is nuanced and context-dependent.

Who May Find This Useful

This discussion may be of interest to students and enthusiasts of quantum mechanics, particularly those seeking to understand the implications of the Heisenberg uncertainty principle and its applications in experimental contexts.

fluidistic
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[tex]\Delta E \Delta t \geq \frac{\hbar}{2}[/tex].
If I understand well, if I measure the energy of a particle (or system of particles) with a great precision, I cannot know well at all when the system had this energy... right?

My doubt is: The system had (or will have?!) the energy I measured, but when? Well, it could be long ago, a few seconds ago, or... in the future?
I don't really know how to form my question.
Say I measure with a 100% accuracy the energy of a particle. I will have a 0% accuracy in the time the system had this energy. However I know it can't be in future (right?), so there's a restriction in time. It can only be present or past, but not future... unless I'm wrong.
My common sense tells me I can't measure an energy the system never had if I measured with a perfect accuracy (or almost perfect). However from Heisenberg principle, all seems to indicate that I can measure very accurately an energy that the system will have within say [tex]10 ^9[/tex] years, which makes no sense to me.

Can someone explain clear my doubts?
In a sketch, say I have the "time axis" on the real numbers. Delta t would be an interval. On another real line I could put the value I measured for the energy. The interval being very small or even vanishing if I measured perfectly. So I know "the" value of the energy of the system. In this case, the Delta t interval would be the whole real numbers axis. However if the positive t's means future, I know I can't have measured the energy the system will be in the future! So I can reduce the interval from [tex]-\infty[/tex] to [tex]0[/tex]. And so writing [tex]\Delta E \Delta t \geq \frac{\hbar}{2}[/tex] is wrong although [tex]\Delta x \Delta p \geq \frac{\hbar}{2}[/tex] is correct.

I hope you can understand what I mean. In case not, I'll try to clarify but please let me know.
 
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If [tex]\Delta E=0[/tex], which means that the state of the system is some energy eigenstate, then [tex]\Delta t=\infty[/tex] and these means that the system will remain stationary (no changes in the state of the system).

But if [tex]\Delta E\neq 0[/tex], for example the system is in superposition of two energy eigenstates: [tex]\psi=c_1 \psi_1+\psi=c_2 \psi_2[/tex], then [tex]\Delta t[/tex] is finite which means that the state of the system is not stationary, it will evolve in time: [tex]\psi(t)=c_1 \psi_1 exp(-iE_1 t/\hbar)+c_2 \psi_2 exp(-iE_2 t/\hbar)[/tex].

So [tex]\Delta t[/tex] is actually the time we need to wait for some reasonable change in the state of the system.
 
Last edited:
Ummmm,

The problem with quantum mechanics is that the classes are not taught with an emphasis on experimental methods. To answer your question

1) I'm not sure you can directly measure the energy of a particle.

2) You can probe the momentum of a free particle and calculate the energy... using a magnetic field and measuring deflection, or using scintillators?

2) Or you can probe the energy absorbed or emitted during some transition. The is a measurement of DE

3) I think your question would be readily answered if you could come up with some experiment, that describes how the quantities are measured.
 
maxverywell said:
So [tex]\Delta t[/tex] is actually the time we need to wait for some reasonable change in the state of the system.
I'm all confused on the meaning of [tex]\Delta t[/tex]. Is it what you say, i.e. it's the time needed for the system to change its state (I don't even know what a state is yet)?
Or is it a time interval like [tex][t_1, t_2][/tex] where the present time is in the middle of the interval?
Or both meanings?

I'll try to rephrase my original doubt: If I measure with a good accuracy [tex]\Delta E[/tex], I will get a large value for [tex]\Delta t[/tex]. Since \Delta t include both past and future (and even present), can I simply discard half of the interval [tex]\Delta t[/tex], namely the future?






Iforgot said:
Ummmm,

The problem with quantum mechanics is that the classes are not taught with an emphasis on experimental methods. To answer your question

1) I'm not sure you can directly measure the energy of a particle.

2) You can probe the momentum of a free particle and calculate the energy... using a magnetic field and measuring deflection, or using scintillators?

2) Or you can probe the energy absorbed or emitted during some transition. The is a measurement of DE

3) I think your question would be readily answered if you could come up with some experiment, that describes how the quantities are measured.
You might be right. My understanding is that in practice is that [tex]\Delta E \Delta t > \frac{\hbar}{2}[/tex] while in theory it could be [tex]\Delta E \Delta t = \frac{\hbar}{2}[/tex] if I can get the best measure ever.
But since I've been thrown the formulas without any explanation (not even how to derive them, yet), I certainly has almost no understanding of it.
 
I just found in Pfeffer's book "Modern Physics, an introductory text"

Pfeffer said:
In general, if the energy of an excited stationary state is accurately determined, as it usually can be by spectroscopic measurements of the frequency of the photons emitted in transitions from it, no accurate information can be obtained as to the moment the individual photons were actually emitted.
which seems to confirm that I can really discard any t in the future!
Therefore [tex]\Delta t[/tex] can't be the whole real axis. In the worst case I can measure very, very accurately the energy of a particle, but I can't know well at all when the particle had this energy. However, I know that it couldn't have it "before the big bang" and I also know it can't be in the future, therefore the worst [tex]\Delta t[/tex] would be around [0, today] where 0 means the big bang's time.
So it's impossible that [tex]\Delta t \to +\infty[/tex]!
 
The time-uncertainty uncertainty principle is not a true uncertainty relation; time is not an operator. The equation posted holds, but only in some specific circumstances. (there's been quite a few threads about this)

For more information, check out http://arxiv.org/abs/quant-ph/0609163" (from a PF contributor no less)
 
Last edited by a moderator:
alxm said:
The time-uncertainty uncertainty principle is not a true uncertainty relation; time is not an operator. The equation posted holds, but only in some specific circumstances. (there's been quite a few threads about this)

For more information, check out http://arxiv.org/abs/quant-ph/0609163" (from a PF contributor no less)

Well, thanks a lot. Although I can't understand everything on the topic yet, I get the main idea and that there's a big difference between saying [tex]\Delta x \Delta p \geq \frac{\hbar}{2}[/tex] and [tex]\Delta E \Delta t \geq \frac{\hbar}{2}[/tex].
By the way do you know if the author of the paper is a Ph.D.? Or at least that the paper is not crackpotry? I'll be studying QM in the next semester so I can't really judge the paper and I don't want to learn false facts; although I'd love to fully understand the whole paper as it can clear many doubts I believe.
 
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Is it helpful to imafine ΔΕ as energy fluctuation and Δt the time a process lasts?
 
woodyallen1 said:
Is it helpful to imafine ΔΕ as energy fluctuation and Δt the time a process lasts?

I don't think so... why would it be?!
 
  • #10
Imagine ΔΕ as an energy loan. The shortest the process is the bigger the loan is.
 
  • #11
That's one way to think of it.

An example of this working is with lifetimes of electronic excitation states. If a state has a very short lifetime (Δt), the energy it emits will be distributed quite widely (i.e. if you try to measure the energy of the state, your sigma will be quite large), whereas a state with a really long lifetime will give you a distribution that is very peaked, meaning small ΔE.
 
  • #12
fluidistic said:
I'll be studying QM in the next semester so I can't really judge the paper and I don't want to learn false facts; although I'd love to fully understand the whole paper as it can clear many doubts I believe.

The author of the article is a theoretical physicist and the article itself appeared in the journal Foundations of Physics in 2007. On this board he is one of the most respected contributors to the quantum physics forum on this board. He has his own opinions on the subject, but these opinions come from a deep knowledge of the subject.

I have to say I'm a big fan of that article, I felt that it was written in such an easy to digest way and I also felt it genuienly improved my understanding of some ideas I had not previously been able to wrap my head around fully. The only very tiny criticism I have is that the pedant in me says you should always use 'spatial' instead of 'spacial', but that really is just pedantry!
 

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