Mathematics – Logic
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006an....327..429k&link_type=abstract
Astronomische Nachrichten, Vol.327, Issue 5/6, p.429
Mathematics
Logic
Magnetic Fields, Cosmology: Theory, Cosmology: Large-Scale Structure, Galaxies: Formation, Galaxies: Clusters: General
Scientific paper
If a magnetic field, B, is frozen into a plasma that undergoes spherical compression then B varies with the plasma density ρ according to B ∝ ρ2/3. In the gravitational collapse of cosmological density perturbations, however, quasi-spherical evolution is very unlikely. In anisotropic collapses the magnetic field can be a much steeper function of gas density than in the isotropic case. We investigate the distribution of amplifications in realistic gravitational collapses from Gaussian initial fluctuations using the Zel'dovich approximation. Representing our results using a relation of the form B ∝ ρα, we show that the median value of α can be much larger than the α=2/3 resulting from spherical collapse, even if there is no initial correlation between magnetic field and principal collapse directions.
Coles Peter
King Emma J.
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