arXiv · cond-mat/0101219
The exact renormalization group in Astrophysics
Abstract
The coarse-graining operation in hydrodynamics is equivalent to a change of scale which can be formalized as a renormalization group transformation. In particular, its application to the probability distribution of a self-gravitating fluid yields an "exact renormalization group equation" of Fokker-Planck type. Since the time evolution of that distribution can also be described by a Fokker-Planck equation, we propose a connection between both equations, that is, a connection between scale and time evolution. We finally remark on the essentially non-perturbative nature of astrophysical problems, which suggests that the exact renormalization group is the adequate tool for them.
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Jose Gaite. 2001-01-15. The exact renormalization group in Astrophysics. https://doi.org/10.1142/s0217751x01004670
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