Classical Version of Vacuum Polarization

In summary, the vacuum polarization result in QED can be written in a "QED form" or an old-fashioned classical physics form. The classical form would include a function f(r) that deviates from the inverse distance squared non-QED function. This function can be expressed as g(r), where g(r) is a normal function. The basic equation for the vacuum polarization correction potential was first derived by Uehling and extends out to about 1 electron Compton wavelength. The correction is a large one and can impact atomic binding energies significantly. The Uehling integral has been rewritten in a more useful integrable form by Shafer.
  • #1
ApplePion
189
0
The vacuum polarization result in QED seems to always be written in a "QED form". I would be interested in seeing it in an old-fashioned classical physics form.

Without vacuum polarization the electric potential in a region containing a point charge is of course Q/r. So if the vacuum polarization is included the potential must be of some form Q f(r) where f(r) is no longer 1/r. So what specifically would f(r) be?

Thanks.
 
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  • #2
But classical physics doesn't predict any vacuum polarisation...

So how can we find a function which is non existent??

i failed to understand your question probably...
 
  • #3
Yes, I realize that classical physics does not fully predict the phenomenon, but the pairs whose creation was predicted by QED do produce electric fields in accordance with the rules for electric field generation. More important though is that one should be able to in principle do an actual physical experiment--take a point charge and actually measure the electric field around it. Doing the experiment one would get actual numerical data to construct the field as a function of position. What you would get would deviate from the inverse distance squared non-QED function. So what I want to know is what the actual function would be. There IS some function, and it should be expressable in the form E = g(r), where g(r) is a normal function!
 
  • #4
ApplePion said:
The vacuum polarization result in QED seems to always be written in a "QED form". I would be interested in seeing it in an old-fashioned classical physics form.

Without vacuum polarization the electric potential in a region containing a point charge is of course Q/r. So if the vacuum polarization is included the potential must be of some form Q f(r) where f(r) is no longer 1/r. So what specifically would f(r) be?

Thanks.

I don't understand.
Polarization just masks some of the charge.
the potential equation should be the same.
Shouldnt it?
 
  • #5
The basic equation for the vacuum polarization correction potential was first derived by Uehling in Phys Rev 48, page 55 (1935). The correction (shielding of the bare charge) extends out to about 1 electron Compton wavelength, so it is a large (often over 1%) correction to atomic binding energies in pionic and muonic atoms.

The Uehling integral is rewritten in a more useful integrable form in Appendix B of Shafer "Pion Mass Measurement..." Phys Rev 163 page 1451 (1967).

Bob S
 
  • #6
Excellent answer, Bob S.

Thanks.
 

1. What is the Classical Version of Vacuum Polarization?

The Classical Version of Vacuum Polarization refers to a phenomenon in quantum field theory where virtual particles, which constantly pop in and out of existence in a vacuum, can affect the behavior of external electric fields.

2. How does the Classical Version of Vacuum Polarization differ from the Quantum Version?

The Classical Version of Vacuum Polarization is a simplified, non-quantum description of the effects of virtual particles on external fields. In the Quantum Version, the effects are described using more complex mathematical equations and take into account the uncertainty principle.

3. What is the significance of the Classical Version of Vacuum Polarization?

The Classical Version of Vacuum Polarization is important because it helps us understand the behavior of electric fields in a vacuum and how they are affected by virtual particles. This phenomenon has implications in various fields of physics, such as cosmology and particle physics.

4. Can the Classical Version of Vacuum Polarization be observed in experiments?

No, the effects of the Classical Version of Vacuum Polarization are very small and can only be observed in extremely strong electric fields. In most cases, the effects are only noticeable in theoretical calculations.

5. How does the Classical Version of Vacuum Polarization relate to the concept of vacuum energy?

The Classical Version of Vacuum Polarization is often used in the context of vacuum energy, as virtual particles are seen as a manifestation of the energy of the vacuum. However, the Classical Version does not fully explain the concept of vacuum energy and is only one aspect of it.

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