arXiv · hep-th/9212021
Magnetic Fields and Passive Scalars in Polyakov's Conformal Turbulence
Abstract
Polyakov has suggested that two dimensional turbulence might be described by a minimal model of conformal field theory. However, there are many minimal models satisfying the same physical inputs as Polyakov's solution (p,q)=(2,21). Dynamical magnetic fields and passive scalars pose different physical requirements. For large magnetic Reynolds number other minimal models arise. The simplest one, (p,q)=(2,13) makes reasonable predictions that may be tested in the astrophysical context. In particular, the equipartition theorem between magnetic and kinetic energies does not hold: the magnetic one dominates at larger distances.
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G. Ferretti, Z. Yang. 1992-12-03. Magnetic Fields and Passive Scalars in Polyakov's Conformal Turbulence. https://doi.org/10.1209/0295-5075%2F22%2F9%2F001
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