The origin of large scale magnetic fields in galaxies.

Mathematics – Logic

Scientific paper

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Magnetic Fields: Galaxies, Magnetic Fields: Origin, Galactic Dynamo, Turbulence, Magnetic Fields

Scientific paper

Magnetic fields correlated on several kiloparsec scales are seen in spiral galaxies. Their origin could be due to the winding up of a primordial cosmological field or due to amplification of a small seed field by a turbulent galactic dynamo. Both these options have difficulties. There is no known mechanism for producing the required primordial field. At the same time the turbulent dynamo may self-destruct before being able to produce the large scale field, due to excess of small scale power. The current status of these difficulties is discussed.

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