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The Boltzmann Transport Equation

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Transport Processes in Space Physics and Astrophysics

Part of the book series: Lecture Notes in Physics ((LNP,volume 918))

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Abstract

The non-relativistic Boltzmann equation is given by

$$\displaystyle\begin{array}{rcl} \frac{\partial f} {\partial t} +\boldsymbol{ v} \cdot \nabla _{\boldsymbol{r}}f + \frac{\boldsymbol{F}} {m} \cdot \nabla _{\boldsymbol{v}}f = \left (\frac{\delta f} {\delta t} \right )_{coll},& &{}\end{array}$$
(2.1)

where \(\boldsymbol{r},\boldsymbol{v}\), and t are independent variables.

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Notes

  1. 1.

    A root or zero, x i , of a function g(x) is defined such that g(x i ) = 0, i.e., the function vanishes at x i .

References

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Dosch, A., Zank, G.P. (2016). The Boltzmann Transport Equation. In: Transport Processes in Space Physics and Astrophysics . Lecture Notes in Physics, vol 918. Springer, Cham. https://doi.org/10.1007/978-3-319-24880-6_2

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