Literature DB >> 15600522

Nonlinear theory of a "shear-current" effect and mean-field magnetic dynamos.

Igor Rogachevskii1, Nathan Kleeorin.   

Abstract

The nonlinear theory of a "shear-current" effect in a nonrotating and nonhelical homogeneous turbulence with an imposed mean velocity shear is developed. The shear-current effect is associated with the W x J term in the mean electromotive force and causes the generation of the mean magnetic field even in a nonrotating and nonhelical homogeneous turbulence (where W is the mean vorticity and J is the mean electric current). It is found that there is no quenching of the nonlinear shear-current effect contrary to the quenching of the nonlinear alpha effect, the nonlinear turbulent magnetic diffusion, etc. During the nonlinear growth of the mean magnetic field, the shear-current effect only changes its sign at some value B (*) of the mean magnetic field. The magnitude B (*) determines the level of the saturated mean magnetic field which is less than the equipartition field. It is shown that the background magnetic fluctuations due to the small-scale dynamo enhance the shear-current effect and reduce the magnitude B (*) . When the level of the background magnetic fluctuations is larger than 1/3 of the kinetic energy of the turbulence, the mean magnetic field can be generated due to the shear-current effect for an arbitrary exponent of the energy spectrum of the velocity fluctuations.

Year:  2004        PMID: 15600522     DOI: 10.1103/PhysRevE.70.046310

Source DB:  PubMed          Journal:  Phys Rev E Stat Nonlin Soft Matter Phys        ISSN: 1539-3755


  1 in total

1.  Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF.

Authors:  Piyush Sharda; Christoph Federrath; Mark R Krumholz; Dominik R G Schleicher
Journal:  Mon Not R Astron Soc       Date:  2021-02-25       Impact factor: 5.287

  1 in total

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