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2.1.3 Dimensional Reduction

To derive a numerically tractable model from the full (3+3)-dimensional Boltzmann equation we assume that the distribution $ f({\mathbf{x}},{\mathbf{k}})$ is one-dimensional in space $ {\mathbf{x}}$ and has cylinder symmetry in $ {\mathbf{k}}$. That is

$\displaystyle f({\mathbf{x}},{\mathbf{k}}) = f(x_3,k_3,k_r),$   where$\displaystyle \quad k_r^2 = k_1^2 + k_2^2   .$ (2.11)

This is known as the ``1+2''-Boltzmann equation. Note that also the input data has to fulfill this symmetry. Consequently the cylinder radial components of the electrical field $ E$ vanish.

With this assumption we have

$\displaystyle \frac{\partial f}{\partial x_1} = \frac{\partial f}{\partial x_2} = 0$ (2.12)

and

$\displaystyle E_{x_1} = E_{x_2} = 0   .$ (2.13)

Hence the BTE reduces for parabolic bands to

$\displaystyle \frac{\partial f}{\partial t} + v_3 \cdot \nabla_{x_3} f + \frac{q}{m^{*}} E_{x_3} \cdot \nabla_{v_3} f = Q(f)   .$ (2.14)

previous up next contents Previous: 2.1.2 Poisson Equation Up: 2.1 The Boltzmann Poisson Next: 2.1.4 Distribution Function Models


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