| Issue |
EAS Publications Series
Volume 32, 2008
Stellar Nucleosynthesis: 50 years after B2FH
|
|
|---|---|---|
| Page(s) | 81 - 130 | |
| DOI | https://doi.org/10.1051/eas:0832003 | |
| Published online | 06 November 2008 | |
Stellar Nucleosynthesis: 50 years after B2FH
C. Charbonnel and J.-P. Zahn (eds)
EAS Publications Series, 32 (2008) 81-130
C. Charbonnel and J.-P. Zahn (eds)
EAS Publications Series, 32 (2008) 81-130
Transport Processes in Stars: Diffusion, Rotation, Magnetic fields and Internal Waves
Département de Physique, Université de Montréal, CP 6128,
succursale centre-ville, Montréal, Québec, H3C 3J8
In this paper, I explore various transport processes that have a large impact of the distribution of elements inside stars and thus, on stellar evolution. A heuristic description of the physics behind equations is provided, and key references are given. Finally, for each process, I will briefly review (some) important results as well as discuss directions for future work.
© EAS, EDP Sciences, 2008