As often used before each volume element \(dk\) contains
| \begin{equation*} 2 \frac{d^3k}{(2\pi)^3} \end{equation*} | (5.19) |
electronic states which are occupied with
| \begin{equation*} dn = \frac{d^3k}{4\pi^3} f(\vec{r},\vec{k}) \end{equation*} | (5.20) |
particles. The complete current density is therefor
Here we used
| \begin{equation*} \int_{V_k} \vec{v}(\vec{k}) f_0(\vec{r},\vec{k}) d^3k = 0 \end{equation*} | (5.22) |
since \(f_0(\vec{r},\vec{k})\) is a symmetric function in \(\vec{k}\), \(\vec{v}\) an antisymmetric function in \(\vec{k}\) and we integrate over symmetric boundaries (In equilibrium no currents are flowing!). Correspondingly we find for the energy flux density:
| \begin{equation*} W = \frac{1}{4\pi^3}\int_{V_k} E(\vec{k})\vec{v}(\vec{k}) f^{(1)}(\vec{r},\vec{k}) d^3k \qquad . \end{equation*} | (5.23) |
© J. Carstensen (Stat. Meth.)