Identity with Gamma matrices and four-vector contractions

In summary, the proof for the generic four-vector "q" being correct is based on the defining property of the ##\gamma## matrices, which can be written as (with the Einstein summation convention in action) $$q_{\alpha} q_{\beta} \gamma^{\alpha} \gamma^{\mu} \gamma^{\beta}=2q_{\alpha} \gamma^{\alpha} q^{\mu} - q^2 \gamma^{\mu}.$$ Additionally, there is no equivalent of "slashed" from the LaTeX package slashed.sty to type "Feynman slashes".
  • #1
Francisco Alegria
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TL;DR Summary
I want to determine a specific identity involving gamma matrix and four vectors
Is the fowwowin identity correct for a generic four-vector"q"? What is the proof? Thank you.
Quantum Physics Identity with Gamma matrices.png
 
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  • #2
That's "Diracology". You need the defining property of the ##\gamma## matrices,
$$\{\gamma^{\mu},\gamma^{\nu} \}=2 \eta^{\mu \nu}.$$
Your expression can be written as (with the Einstein summation convention in action)
$$\begin{split}
q_{\alpha} q_{\beta} \gamma^{\alpha} \gamma^{\mu} \gamma^{\beta}&=q_{\alpha} q^{\beta} \left (\gamma^{\alpha} \{\gamma^{\mu},\gamma^{\beta} \} - \gamma^{\alpha} \gamma^{\beta} \gamma^{\mu} \right) \\ &= q_{\alpha} q_{\beta} \left (2\gamma^{\alpha} \eta^{\mu \beta} - \frac{1}{2} \{\gamma^{\alpha} ,\gamma^{\beta} \} \gamma^{\mu} \right)\\
&=2q_{\alpha} \gamma^{\alpha} q^{\mu} - q^2 \gamma^{\mu}.
\end{split}$$
[Note: Is there some equivalent of "slashed" from the LaTeX package slashed.sty to type "Feynman slashes"?]
 
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  • #3
vanhees71 said:
[Note: Is there some equivalent of "slashed" from the LaTeX package slashed.sty to type "Feynman slashes"?]
##\not{\!p}## is produced by typing "\not{\!p}".
 
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FAQ: Identity with Gamma matrices and four-vector contractions

What are Gamma matrices in the context of quantum field theory?

Gamma matrices are a set of matrices used in the formulation of the Dirac equation, which describes the behavior of fermions such as electrons. They are elements of the Clifford algebra and are used to represent the spinor fields in relativistic quantum mechanics. The most common set of Gamma matrices are the Dirac matrices, which are used to linearize the Klein-Gordon equation.

How do Gamma matrices relate to four-vectors in relativistic quantum mechanics?

In relativistic quantum mechanics, four-vectors are used to represent quantities like position, momentum, and current in spacetime. Gamma matrices are used to construct bilinear covariants, which are scalar quantities formed by the contraction of spinor fields with Gamma matrices and four-vectors. This allows for the formulation of Lorentz-invariant quantities, which are essential for maintaining the consistency of physical laws in all inertial frames.

What is the significance of the identity involving Gamma matrices and four-vector contractions?

The identity involving Gamma matrices and four-vector contractions is significant because it simplifies the calculations in quantum field theory. These identities often involve trace theorems and commutation relations that reduce complex expressions into more manageable forms. This is particularly useful in Feynman diagram calculations and in proving the invariance of physical quantities under Lorentz transformations.

Can you provide an example of an identity involving Gamma matrices and four-vector contractions?

One common identity is the Fierz identity, which relates products of Gamma matrices to sums of other Gamma matrices. For example, a simple Fierz identity in four-dimensional spacetime is given by: \[ (\gamma^\mu)_{\alpha\beta} (\gamma_\mu)_{\gamma\delta} = 2 \delta_{\alpha\delta} \delta_{\beta\gamma} - \delta_{\alpha\beta} \delta_{\gamma\delta} \]This identity is used to simplify expressions involving the contraction of Gamma matrices with four-vectors and spinor fields.

How are these identities used in practical calculations in quantum field theory?

These identities are used in practical calculations to simplify the evaluation of Feynman diagrams, which represent interactions between particles. For example, in calculating scattering amplitudes, one often encounters traces of products of Gamma matrices. Using identities involving Gamma matrices and four-vector contractions, these traces can be reduced to simpler forms, making the computation of physical observables like cross-sections and decay rates more tractable.

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