Magnetic amplification in cylindrical cosmological structure

Astronomy and Astrophysics – Astrophysics

Scientific paper

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10 pages, 4 figures included; accepted to A&A

Scientific paper

10.1051/0004-6361:20035595

We derive the amplification of the cosmological magnetic field associated
with forming gravitational structure. The self-similar solutions of
magnetohydrodynamic equations are computed both in linear and nonlinear
regimes. We find that the relatively fast magnetic field enhancement becomes
substantial in the nonlinear phase.

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