Covariance of the Dirac equation and Infinitesimal Lorentz transformation Okay, I've got really desperate now. I've spend 10 hours of work (for a few days) trying to prove 'trivial' equation in Quantum Electrodynamics. To anybody who want to write an answer for my questions - treat me like an idiot who only can multiplicate and sum equations. NO HYPERLINKS (I know how to use Google and sources, really!), NO SHORTCUTS. Please, it's very important to me.
So, main question is:
Let's suppose Lorentz transformation: $\Lambda^a_b=g^a_b+\Delta\omega^a_b$, where $\Delta\omega^a_b$ is just a (small) number ($\Delta\omega^2$ can be neglected). So, we can build an equation for transformation matrix S:
$S^{-1}\gamma^iS=\Lambda^i_j\gamma^j$
where $\gamma^i$ are Dirac matrix (you know, these fundamental in Dirac Equation). It is now easy to show that S:
$S=I+iS^{ab}\Delta\omega_{ab}$
$S^{-1}=I-iS^{ab}\Delta\omega_{ab}$
Something like that. $\Delta\omega$ is still a number, but $s$ is a matrix. Now black magic happens and we get:
$S^{ab} = \frac{i}{4}\big[\gamma^a,\gamma^b\big]$
In some like 5 sources proof of last equation is described as 'trivial' or as 'exercise for reader'. If my explanation is too much complicated, here is a short one:


*

*Read a http://physics.ucsd.edu/students/courses/fall2009/physics130b/Dirac_Lorentz.pdf script

*Go to page 26 (in pdf, at page numerated by page 22)

*Prove equation (46).

 A: The direct sum of $\left(\frac{1}{2}, 0\right), \left(0, \frac{1}{2}\right)$ gives the Dirac bispinor $\Psi $ with components $\psi_{a}, \kappa_{\dot {a}}$. Here there is the infinitesimal transformation law for them:
$$
\delta \psi_{a} = \frac{i}{2}\omega^{\mu \nu}(J_{\mu \nu})_{a}^{\quad b}\psi_{b}, \quad \delta \kappa_{\dot {a}} = \frac{i}{2}\omega^{\mu \nu}(J_{\mu \nu})_{\dot {a}}^{\quad \dot {b}}\kappa_{\dot {b}}, \qquad (.1)
$$
where $(J_{\mu \nu})_{a}^{\quad b}$ is the generator of the Lorentz group in spinor representation. They are given by
$$
(J_{\mu \nu})_{a}^{\quad b} = -i(\sigma_{\mu \nu})_{a}^{\quad b}, \quad (J_{\mu \nu})_{\dot {a}}^{\quad \dot {b}} = -i(\tilde {\sigma}_{\mu \nu})_{a}^{\quad b}, \qquad (.2)
$$
where
$$
(\sigma^{\mu \nu})_{\alpha \beta } = -\frac{1}{4}\left( (\sigma^{\mu}\tilde {\sigma}^{\nu})_{\alpha \beta} - (\sigma^{\nu}\tilde {\sigma}^{\mu})_{\alpha \beta }  \right), \quad (\tilde {\sigma}^{\mu \nu})_{\dot {\alpha } \dot {\beta }} = -\frac{1}{4}\left( (\tilde {\sigma}^{\mu}\sigma^{\nu})_{\dot {\alpha } \dot {\beta } } - (\tilde {\sigma }^{\nu}\sigma^{\mu})_{\dot {\alpha }  \dot {\beta } }  \right) ,
$$
$$
\tilde {\sigma}^{\mu} = (\hat {\mathbf E}, -\hat {\mathbf \sigma}) .
$$
This is the most untrivial part of the derivation.
So, after substitution $(.2)$ to $(.1)$, you can get
$$
\delta \psi_{a} = \frac{1}{2}\omega^{\mu \nu}(\sigma_{\mu \nu})_{a}^{\quad b}\psi_{b}, \quad \delta \kappa_{\dot {a}} = \frac{1}{2}\omega^{\mu \nu}(\tilde {\sigma }_{\mu \nu})_{\dot {a}}^{\quad \dot {b}}\kappa_{\dot {b}} \Rightarrow
$$
$$
\delta \Psi = \delta (\psi_{a} \quad \kappa_{\dot {a}})^{T}= \frac{\omega^{\mu \nu}}{2}\begin{pmatrix} \sigma_{\mu \nu} & 0 \\ 0 & \tilde {\sigma }_{\mu \nu} \end{pmatrix}\Psi . \qquad (.3)
$$
Then you can introduce gamma-matrices and their combination:
$$
\gamma_{\mu} = \begin{pmatrix} 0 & \sigma_{\mu} \\ \tilde {\sigma}_{\mu} & 0 \end{pmatrix}, \quad S_{\mu \nu} = \frac{1}{4}\left( \gamma_{\mu}\gamma_{\nu} - \gamma_{\nu }\gamma_{\mu} \right) = \begin{pmatrix} \sigma_{\mu \nu} & 0 \\ 0 & \tilde {\sigma }_{\mu \nu} \end{pmatrix},
$$
and so, by using $(.3)$, you can straightforward get the wanted result
$$
 \delta \Psi = \frac{\omega^{\mu \nu}}{2}S_{\mu \nu}\Psi .
$$
Of course, this matrix and transformation law is also applicable for the transformations of $\gamma$-matrices.
