Inverse cascades and primordial magnetic fields

P Olesen - Physics Letters B, 1997 - Elsevier
Physics Letters B, 1997Elsevier
We consider primordial spectra with simple power behaviours and show that in the Navier-
Stokes and magnetohydrodynamics equations without forcing, there exists systems in three
dimensions with a subsequent inverse cascade, transferring energy from small to large
spatial scales. This can have consequences in astrophysics for the evolution of density
fluctuations, for primordial magnetic fields, and for the effect of diffusion. In general, if the
initial spectrum is kα, then in the “inertial” range, for α>− 3 there is an inverse cascade …
We consider primordial spectra with simple power behaviours and show that in the Navier-Stokes and magnetohydrodynamics equations without forcing, there exists systems in three dimensions with a subsequent inverse cascade, transferring energy from small to large spatial scales. This can have consequences in astrophysics for the evolution of density fluctuations, for primordial magnetic fields, and for the effect of diffusion. In general, if the initial spectrum is kα, then in the “inertial” range, for α > −3 there is an inverse cascade, whereas for α < −3 there is a forward cascade.
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