Covariant Uncertaintly Principle

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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.
 
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).
 
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?
 


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.