Abstract
The non-relativistic Boltzmann equation is given by
where \(\boldsymbol{r},\boldsymbol{v}\), and t are independent variables.
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Notes
- 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
Gombosi, T.I.: Physics of the Space Environment. Cambridge Atmospheric and Space Science Series. Cambridge University Press, Cambridge (1998)
Gradshteyn, I.S., Ryzhik, I.M.: Table of Integrals, Series, and Products, 7th edn. Academic Press, New York (2000)
Melrose, D.B., Pope, M.H.: Proc. Astron. Soc. Aust. 10, 222 (1993)
Schlickeiser, R.: Cosmic Ray Astrophysics. Springer, Berlin (2002)
Zank, G.P.: Transport Processes in Space Physics and Astrophysics. Lecture Notes in Physics, vol. 877, 1st edn. Springer, New York (2014)
Zank, G.P., Matthaeus, W.H., Smith, C.W.: J. Geophys. Res. 101, 17093 (1996). doi:10.1029/96JA01275
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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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DOI: https://doi.org/10.1007/978-3-319-24880-6_2
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