Physics Asked on August 14, 2021
While going through the third chapter of Peskin’s QFT book, I am stuck at the following proof:
$$[gamma^mu, S^{rhosigma}] = (mathcal{J}^{rhosigma})^mu_{~nu} gamma^nu,$$
where,
$$S^{munu} = frac{i}{4} [gamma^mu, gamma^nu]qquad;qquadqquad(mathcal{J}^{munu})_{alphabeta} = i (delta^mu_alpha delta^nu_beta – delta^mu_beta delta^nu_alpha).$$
Using these above definitions, I found from R.H.S. of the first equation,
$$(mathcal{J}^{rhosigma})^mu_{~nu} gamma^nu = i (delta^{rhomu} gamma^sigma – delta^{sigmamu} gamma^rho)$$
and from L.H.S. of the first equation,
$$[gamma^mu, S^{rhosigma}] = i (g^{rhomu} gamma^sigma – g^{sigmamu} gamma^rho).$$
Clearly there is a big difference between the two sides. One side has the metric tensors, whereas other side has delta functions. I think this will be fine if in the definition of $(mathcal{J}^{munu})_{alphabeta}$ the delta functions are replaced by the metric tensors. It would be great if anyone could shade some light on this.
You forgot to lower the $mu$ index in ${(mathcal{J}^{rhosigma})^mu}_nu$ before using its definition. Doing it makes $g$ appear as you need.
Answered by Emmy on August 14, 2021
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