At what scale is the charge of an electron -2e?

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Discussion Overview

The discussion centers around the charge of an electron and its behavior at various energy scales, particularly exploring the conditions under which the charge may be observed as -2e. Participants delve into theoretical aspects of quantum field theory, perturbation theory, and the running of the fine structure constant.

Discussion Character

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

Main Points Raised

  • One participant asserts that the charge of an electron is -e at atomic scales but becomes infinite at infinitesimal scales, suggesting a continuous relation for renormalization.
  • Another participant challenges the claim about infinite charge at infinitesimal scales, stating that the coupling strength is scale-dependent and does not become infinite below the Planck scale.
  • A participant proposes a formula relating bare charge to coupling strength and seeks to determine the scale at which the coupling strength equals 2.
  • Participants discuss the running of the fine structure constant with energy scale, referencing specific values at different energy levels and questioning the accuracy of provided values.
  • One participant expresses difficulty in applying a formula for the fine structure constant and presents calculations that yield different results than expected.
  • Another participant suggests that the discrepancy in values may indicate an error in the original reference, comparing it with a plot that supports a different value.
  • A participant derives a relationship for Q in terms of the fine structure constant and suggests a scale significantly larger than the Planck energy, raising questions about the appearance of higher order terms.
  • Further discussion includes the nature of higher order terms and their relevance below the Planck scale, as well as a brief inquiry into the concept of a Z-pole.
  • One participant notes that QED becomes less useful at energy scales significantly larger than the Higgs vacuum energy, indicating a shift to a different theoretical framework.

Areas of Agreement / Disagreement

Participants express differing views on the behavior of the electron charge at various scales, particularly regarding the implications of coupling strength and the running of the fine structure constant. The discussion remains unresolved with multiple competing perspectives on these theoretical aspects.

Contextual Notes

Participants highlight limitations in the application of formulas and the dependence on specific definitions, particularly regarding the behavior of the fine structure constant and the implications of energy scales on theoretical models.

utesfan100
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The charge of an electron is -e in energy scales well into the atomic scale. At infinitesimal scales it becomes infinite. This relation must be continuous for re-normalization to work, thus the intermediate value theorem asserts that it attains all values between at some energy level. I want to determine the scale at which the charge is observed to be -2e.

This should only involve a few highest order terms. Where can I find the highest order perturbation terms for the charge of an electron as the energy scale increases/length scale decreases?
 
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utesfan100 said:
At infinitesimal scales it becomes infinite.
Where did you read that, and what does that mean?

The coupling strength, not the charge, is scale-dependent, but it does not get infinite below the Planck scale. And we know our physics doesn't work beyond that.
 
To contextualize your answer I am picturing something like

bare charge = coupling strength * e

in the limit where the length scale goes to infinity.

At what scale, then, is the coupling strength 2?
 
Thank you for the link, but I am having difficulties using the formula provided. When I plug the values you give I don't get the values you give. The formula given is:

α1=α/[1-α/(3π)*log(Q^2/me^2)]

In particular, the log of 0 diverges to -infinity, so at 0 the formula goes to positive 0. That said, it gives a value of 1/138.3 at the energy scale of the CMBR, so it diverges very slowly, and exactly 1/137 at the energy scale of the rest mass of an electron times c^2.

At Q=90GeV≈180,000*me*c^2, I don't get 1/128.

log(180,000^2)=10.51
a/(3π)*10.51=0.00814
1-0.00814=0.99186
1/137/0.99186=1/135.9 ≠ 1/128

Even interpreting the log as ln, as some web references occasionally use, only gets me to 1/134.4.
 
The 128 looks like an error. Compare it with this plot, which agrees with 1/134.4=0.00744, but is clearly inconsistent with 1/128=0.00781.

Natural logarithm.
 
Thank you. So then, solving for Q in terms of α1/α I get:

Q=me*e^[3π/α*(α1/α-1)]≈me*e^[645.6*(α1/α-1)]

For α1/α=2 I get 2E+280me. This appears to answer my question. :)

Before leaving I have two quick follow ups.
1) This is significantly larger than the plank energy. Would I be wrong to think that higher order terms certainly appear before then?
2) What is a Z-pole?
 
utesfan100 said:
1) This is significantly larger than the plank energy. Would I be wrong to think that higher order terms certainly appear before then?
They should follow the square, cube, ... of α/(3π)*log(Q^2/me^2) with some different numerical prefactor. Below the Planck scale, this term is much smaller than one, so higher orders should be smaller.
utesfan100 said:
2) What is a Z-pole?
The pole mass of the Z, roughly 90 GeV.
 
  • #10
utesfan100 said:
Would I be wrong to think that higher order terms certainly appear before then?

QED essentially stops being a useful description of the interaction when energy scale gets significantly larger than Higgs vacuum energy. At those scales, SU(2)xU(1) weak isospin/weak hypercharge is a better description, and you need to concern yourself with their constants and their running, not fine structure constant's running.

Your question, thus, was a theoretical one, about the imaginary Universe where QED is the actual interaction, not a low-energy limit of weak force.
 

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