Physics
Scientific paper
Apr 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..apr.b7005k&link_type=abstract
American Physical Society, April Meeting, April 29-May 2, 2000 Long Beach, CA, abstract #B7.005
Physics
Scientific paper
I will discuss two possible origins for cosmic magnetic fields. First, the origin in the protostructures driven by gravitational instabilities produced by gravitational collapse. I will show that on the basis of a cascade it is possible to produce larges scale strong magnetic fields. These fields can provide the seed fields for galaxies and clusters of galaxies, or even provide a primordial origin for them. Second, I will discuss the classical alpha omega dynamo origin for galactic fields. I will stress a major difficulty with them. Namely, the necessity for these dynamos to get rid of flux by expulsion from the galactic disks. I will discuss the major difficulties associated with this expulsion of matter loaded lines of force escaping from the very deep gravitational well. I will finally compare the likelyhood of these two dynamos for the creation of cosmic magnetic fields.
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