Magnetic amplification in cylindrical cosmological structure
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🌌 astro-ph
keywords
magneticamplificationcosmologicalfieldnonlinearstructureassociatedbecomes
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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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