Fermion Anticommutation Relations (nightmare)

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Discussion Overview

The discussion revolves around proving the anticommutation relations for fermionic fields, specifically focusing on equation (5.15) from a set of lecture notes. Participants explore the similarities and differences between the proof of anticommutation relations and the commutation relations previously established in the notes.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant expresses difficulty in proving equation (5.15) and notes that the proof should mirror that of (5.5), with a key difference being a minus sign in the second term.
  • Another participant questions the reliability of the reference, citing different results for scalar fields and providing specific equations for commutation relations.
  • A different participant believes that the relations in (5.15) are correct but expresses uncertainty about the normalization factor for spinors and suggests a method to extract operators using the spinor scalar product.
  • One participant argues that the proof in the notes is flawed, asserting that {ψ(x), ψ†(y)} does not equal a delta function.
  • Another participant asserts that the correct relations for scalar fields differ from those stated, referencing specific equations from a textbook.
  • There is a clarification about the differences in commutation relations for real versus complex scalar fields, with a participant correcting their earlier sign error.
  • Discussion includes the distinction between the invariant function Δ and the operator S for fermionic fields, with emphasis on the additional factors involved in the Dirac case.
  • Participants discuss the conditions under which Δ leads to a delta function, particularly in relation to time derivatives in the context of fermionic fields.
  • One participant acknowledges a misunderstanding regarding the equivalence of certain equations and expresses clarity after further discussion.

Areas of Agreement / Disagreement

Participants exhibit disagreement regarding the correctness of specific equations and the interpretation of the anticommutation relations. Multiple competing views remain on the validity of the references and the relationships between the various equations discussed.

Contextual Notes

There are unresolved questions regarding the normalization of spinors and the specific forms of the equations for different types of fields. The discussion also highlights the dependence on definitions and the conditions under which certain relations hold.

latentcorpse
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Hi. I've been thinking about this proof for over a day now and have reached the point where I can't come up with any new approaches!

I'm trying to prove equation (5.15) in these notes:
http://www.damtp.cam.ac.uk/user/tong/qft/qft.pdf


Just above eqn (5.15) we are told that the proof should be exactly the same as the proof of (5.5) which is done on p107.

I completely understand the proof on p107 for the commutation relations.
When trying to prove the anticommutation relations, the only difference is going to be a minus sign on the second term.

In other words, the proof is the same as on p107 except we have

\{ \psi( \vec{x}), \psi^\dagger \vec{y} \} = \displaystyle\sum_{s} \in \frac{d^3p}{(2 \pi)^3} \frac{1}{2E_{\vec{p}}} \left( u^s( \vec{p} \bar{u}^s(\vec{p}) \gamma^0 e^{i \vec{p} \cdot ( \vec{x}-\vec{y})} + v^s(\vec{p}) \bar{v}^s(\vec{p}) \gamma^0 e^{-i \vec{p} \cdot (\vec{x} - \vec{y})} \right)

This means that if we follow through the next few steps on p107 we arrive at

\int \frac{d^3p}{(2 \pi)^3} \frac{1}{E_{\vec{p}}} ( p_i \gamma^i + m ) \gamma^0 e^{i \vec{p} \cdot ( \vec{x} - \vec{y} )}

and as far as I can tell there is no way to make that into a delta function!


ANY HELP IS GREATLY APPRECIATED!
 
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Do you really trust this reference?? Because other places give different results!

For a scalar field the commutator is usually quoted as [..x, y are 4-vectors..]

[φ(x), φ*(y)] = iΔ(x - y)

where Δ is the "invariant delta function", defined by

iΔ(x) = (2π)-3∫d3k/2ω [e-ik·x - eik·x]

Δ(x) vanishes for equal times, and its time derivative at equal times is a 3-dimensional δ function: (∂Δ(x)/∂x0)|(x0 = 0) = - δ3(x). Notice it is not true that [φ(x), φ*(y)] at equal times is a δ-function.. you must include the time derivative.

The corresponding relation for Dirac spinor fields is

{ψ(x), ψ†(y)} = -iS(x - y)

where

S(x - y) = (iγμμ + m)Δ(x - y)
 
I think relations (5.15) are correct (although I'm not sure for the (2π)^{3} that probably depends on the normalization of u and v spinors). I think you can extract an expression for c and b operators using the spinor scalar product. For example, if I'm not wrong, the following equation should be true:
$$b^{r}_{\vec{p}}=\int{d^3x U^{\dagger}(r\vec{p})\psi(x)}$$
where:

$$U(r\vec{p})=\frac{1}{(2\pi)^{3/2}}\frac{1}{\sqrt{2E_{\vec{p}}}}u^s(\vec{p})e^{-ipx}$$

When you have extract both b and c you can anticommutate them and using the anticommutation relations on ψ and ψ^{+} you should reach your goal.

I hope I'm not wrong, as I'm using my old notes and there should be something different from yours but I think the main idea should be ok.
 
Tong's proof is trying to go the other way. He assumes (5.15) and tries to prove (5.14). But as I indicated above, (5.14) is wrong. {ψ(x), ψ†(y)} is not equal to a delta function.
 
Maybe I'm missing something. Is ψ the fermionic field? If so, I'm quite sure that 5.14 are correct. I think you got wrong when you said that:

$$[\phi(x),\phi^\dagger(y)]=i\Delta(x-y)$$

as the correct relations, for scalar fields, should be:

$$[\phi(x),\dot{\phi}^\dagger(y)]=i\delta^3(\vec{x}-\vec{y})$$
and
$$[\phi(x),\phi(y)]=i\Delta(x-y)$$.

And the same thing is valid for fermionic fields. You can see for example Mandl-Shaw "Quantum Field Theory" equations 3.25 and 3.42.
I hope I'm not wrong, if so I'm sorry :biggrin:
 
Einj, The commutation relations for the Klein-Gordon field are slightly different depending on whether the field is real or complex.

For a real field, [φ(x), φ(y)] = -iΔ(x - y) (Sorry, I had the sign wrong.)

Whereas for a complex scalar field, [φ(x), φ*(y)] = -iΔ(x - y)

Some references call the invariant function D(x -y) instead of Δ(x - y).

Note that your first two equations are equivalent. You can get the second one by taking the time derivative wrt y of the first one, since the equal-time time derivative of Δ(x - y) is δ3(x - y).

And the same thing is valid for fermionic fields.
No, for a Dirac field ψ(x) there's an additional factor: S(x - y) = (iγμμ + m)Δ(x - y). The expression derived by the OP has this factor in it.
 
Ok, I knew that (and of course I said the same thing because S is quite the equivalent of Δ but for fermionic field). However, what should be the fermonic equivalent of my second equation?
 
One big difference between S and Δ: S is a 4 x 4 matrix!

what should be the fermonic equivalent of my second equation?
To get a delta function out of Δ, you need a time derivative. But in the Dirac case, the time derivative is already there, thanks to the (iγμμ + m) in front. At equal times, Δ(x - y) is zero, so all the terms in the definition of S drop out except for the time derivative. You get

{ψ(x), ψ†(y)}|(at x0 = y0) = - γ00Δ(x - y) = γ0 δ3(x - y)

(To leave no doubt about the notation, ψ† is what appears in the bilinear covariants, e.g. jμ = eψ†γμψ.) And so, if you'd rather, using ψ† = ψ*γ0,

{ψ(x), ψ*(y)}|(at x0 = y0) = δ3(x - y)

Maybe this is what Tong had in mind when he wrote (5.14).
 
Ok, understood. Sorry for the misunderstanding.
 

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