Covariant Uncertaintly Principle

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Discussion Overview

The discussion centers around the formulation of the uncertainty principle in a covariant framework, exploring whether it can be expressed as a dot product involving spacetime metrics. Participants examine the implications of this formulation, particularly in the context of relativistic quantum theory and the challenges associated with defining position operators for massless particles like photons.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that the uncertainty principle can be expressed as a dot product using the metric tensor, suggesting formulations like \(\eta^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq\hbar\) or \(g^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq\hbar\).
  • Others question the definitions of \(\Delta x\) and \(\Delta p\), noting the complexities in defining position operators for massless particles, particularly photons.
  • A participant mentions the need for an extended Hilbert space to properly formulate the uncertainty principle and points out a missing factor in the proposed relation for four-dimensional spacetime.
  • There is a discussion about the implications of Lorentzian signature on the uncertainty relation, with one participant suggesting a contraction of terms that is challenged by another participant.
  • Some participants refer to canonical commutation relations as foundational to the uncertainty relation, emphasizing the importance of correctly identifying the canonical momentum associated with position operators.
  • Concerns are raised about the physical consequences of the lack of a position operator for photons, with references to alternative notions of measurable position defined through positive operator-valued measures (POVMs).

Areas of Agreement / Disagreement

Participants express differing views on the formulation of the uncertainty principle and the implications of defining position operators for massless particles. The discussion remains unresolved, with multiple competing perspectives on the validity and interpretation of the proposed formulations.

Contextual Notes

There are limitations in the discussion regarding the assumptions made about the definitions of position and momentum operators, as well as the mathematical steps involved in deriving the proposed relations. The scope of the discussion is primarily focused on theoretical implications rather than experimental validation.

jfy4
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Covariant Uncertainty Principle

Hi,

is it possible to write the uncertainty principle as a dot product like:

[tex]\eta^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq\hbar[/tex]

or even to generalize it as

[tex]g^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq\hbar[/tex]

?
 
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That's not so clear. What's meant by [tex]\Delta x[/tex] and [tex]\Delta p[/tex] here? Note that it is not trivial to define, e.g., position operators for massless particles with spin (e.g., there's no position operator for photons in the strict sense).

You find a good review on the implications of the uncertainty relations in the context of relativistic quantum theory in the beginning of Landau-Lifgarbages vol. IV. This goes back to a famous paper by Bohr.
 
@vanhees71: I'm curious why there's no position operator for photons in the strict sense? Could you explain?
 


jfy4 said:
Hi,

is it possible to write the uncertainty principle as a dot product like:

[tex]\eta^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq\hbar[/tex]
Yes, provided that you work in an extended Hilbert space as in
http://xxx.lanl.gov/abs/0811.1905 [Int. J. Quantum Inf. 7 (2009) 595-602]

But you are missing a factor of D/2=2 for D=4 spacetime dimensions. The correct relation for D=4 is
[tex]\eta^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq 2\hbar[/tex]

jfy4 said:
or even to generalize it as

[tex]g^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq\hbar[/tex]
Yes (with the same correction).
 
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Demystifier said:
Yes, provided that you work in an extended Hilbert space as in
http://xxx.lanl.gov/abs/0811.1905 [Int. J. Quantum Inf. 7 (2009) 595-602]

But you are missing a factor of D/2=2 for D=4 spacetime dimensions. The correct relation for D=4 is
[tex]\eta^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}\geq 2\hbar[/tex]


Yes (with the same correction).

That's curious. When I first wrote it out, I had the 2, but then I thought with the lorentzian signature that the temporal component would subtract one of the the [itex]\hbar/2[/itex]s.

Would it not contract as follows?

[tex]\eta^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}=-\Delta t\Delta E+\Delta x\Delta p_x +\Delta y\Delta p_y +\Delta z\Delta p_z\geq -\frac{\hbar}{2}+\frac{\hbar}{2}+\frac{\hbar}{2}+\frac{\hbar}{2}=\hbar[/tex]
 
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jfy4 said:
That's curious. When I first wrote it out, I had the 2, but then I thought with the lorentzian signature that the temporal component would subtract one of the the [itex]\hbar/2[/itex]s.

Would it not contract as follows?

[tex]\eta^{\alpha\beta}\Delta x_{\alpha}\Delta p_{\beta}=-\Delta t\Delta E+\Delta x\Delta p_x +\Delta y\Delta p_y +\Delta z\Delta p_z\geq -\frac{\hbar}{2}+\frac{\hbar}{2}+\frac{\hbar}{2}+\frac{\hbar}{2}=\hbar[/tex]
No!

You should start from the canonical uncontracted uncertainty relation
[tex]\Delta x^{\alpha}\Delta p_{\beta}=\frac{\hbar}{2} g^{\alpha}_{\beta}[/tex]
and observe that, in any spacetime,
[tex]g^{\alpha}_{\beta}=\delta^{\alpha}_{\beta}[/tex]
 
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Demystifier said:
No!

You should start from the canonical uncontracted uncertainty relation
[tex]\Delta x^{\alpha}\Delta p_{\beta}=\frac{\hbar}{2} g^{\alpha}_{\beta}[/tex]
and observe that, in any spacetime,
[tex]g^{\alpha}_{\beta}=\delta^{\alpha}_{\beta}[/tex]

Interesting.

Where did you find that/How did you know to use that equation (inequality?)? Else, what's wrong with my contraction above?
 


jfy4 said:
Interesting.

Where did you find that/How did you know to use that equation (inequality?)? Else, what's wrong with my contraction above?
Well, the uncertainty relation above is a consequence of

1) The canonical commutation relations
[tex][x^{\alpha},p_{\beta}]=-i\hbar g^{\alpha}_{\beta}[/tex]
which is Eq. (3) in
http://xxx.lanl.gov/abs/0811.1905 [Int. J. Quantum Inf. 7 (2009) 595-602]

and

2) The fact that the canonical momentum associated with [tex]x^{\alpha}[/tex] is [tex]p_{\alpha}[/tex] (not [tex]p^{\alpha}[/tex] as one might naively think).

Your contraction is wrong because it starts from a wrong uncontracted relation. This is related to 2) above.
 
  • #11
kof9595995 said:
Thanks, though I can't really understand the proof.

In a nutshell, the essence of the argument is the following.

A position operator for a spin s particle needs a 2s+1 dimensional spin space.
(Why this is necessary is the most difficult part of the argument.)
This is the case for massive particles. But massless particles only have a 1- or 2-dimensional spin space, depending on whether or not they are chiral.

Photons are not chiral and have spin 1, hence they have only 2 instead of the 3 spin components needed. The missing component would be ''longitudinal'' photons, which do not exist (and cannot for a massless particle).
 
  • #12
A. Neumaier said:
In a nutshell, the essence of the argument is the following.

A position operator for a spin s particle needs a 2s+1 dimensional spin space.
(Why this is necessary is the most difficult part of the argument.)
This is the case for massive particles. But massless particles only have a 1- or 2-dimensional spin space, depending on whether or not they are chiral.

Photons are not chiral and have spin 1, hence they have only 2 instead of the 3 spin components needed. The missing component would be ''longitudinal'' photons, which do not exist (and cannot for a massless particle).

I'm curious what's the physical consequence, does it simply mean we can never measure (or even define?) the position of a photon?
 
  • #13
kof9595995 said:
I'm curious what's the physical consequence, does it simply mean we can never measure (or even define?) the position of a photon?

Not according to the textbook view of measurements. But there are more approximate notions of measurable position, defined in terms of POVMs rather than operators.
http://en.wikipedia.org/wiki/POVM
 
  • #14


Demystifier said:
Well, the uncertainty relation above is a consequence of

1) The canonical commutation relations
[tex][x^{\alpha},p_{\beta}]=-i\hbar g^{\alpha}_{\beta}[/tex]
which is Eq. (3) in
http://xxx.lanl.gov/abs/0811.1905 [Int. J. Quantum Inf. 7 (2009) 595-602]

and

2) The fact that the canonical momentum associated with [tex]x^{\alpha}[/tex] is [tex]p_{\alpha}[/tex] (not [tex]p^{\alpha}[/tex] as one might naively think).

Your contraction is wrong because it starts from a wrong uncontracted relation. This is related to 2) above.

Thanks,

I'll spend some time pondering it over.
 

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