Abstract
Thermonuclear burn in inertial confinement fusion is predicted to involve the most extreme temperatures, densities and pressures ever produced in the laboratory (Lindl et al. in Phys Plasmas 11:339, 2004, [1]).
This chapter is an enhanced version of a chapter from an original PhD thesis which is available Open Access from the repository https://spiral.imperial.ac.uk/ of Imperial College London. The original chapter was distributed under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (http://creativecommons.org/licenses/by-nc-nd/4.0/), which permits any non-commercial use, duplication, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author and the source, provide a link to the Creative Commons license and indicate if you modified the licensed material. You do not have permission under this license to share adapted material derived from this book or parts of it. The Creative Commons license does not apply to this enhanced chapter, but only to the original chapter of the thesis.
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Notes
- 1.
In fact, this scheme is unconditionally stable for the diffusion equation [30].
- 2.
Our scalings here and in the preceding discussion all apply in the ultra-relativistic limit. In the mildly-relativistic case, no simple scaling is possible, as the correction is a product of both the simple physical arguments here, as well as changes to the shape of the distribution function.
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Pike, O.J. (2017). Transport Processes in a Relativistic Plasma. In: Particle Interactions in High-Temperature Plasmas. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-63447-0_4
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