![]() | Annu. Rev. Astron. Astrophys. 1996. 34:
155-206 Copyright © 1996 by Annual Reviews. All rights reserved |
5.2. The Primordial Origin of Galactic Magnetic Fields
We now assess the possibility that the large-scale magnetic field
observed in galaxies is merely a result of the twisting of a cosmological
magnetic field by galactic differential rotation (see e.g.
Kulsrud 1986).
Aiming at conservative estimates, we neglect any magnetic field
dissipation. An isotropic contraction of the protogalaxy with a
frozen-in magnetic field, from an intergalactic density
IG
10-29 g
cm-3 up to an interstellar density
10-24 g
cm-3, results in amplification of the primordial
magnetic field by a factor of 2 × 103. Differential rotation
results in an amplification of the magnetic field in a young galaxy by
the number of galactic rotations in 1010 yr, which is
N ~ 30.
Altogether, a conservative upper limit on the field in the galactic
disk resulting from a primordial field is
![]() |
(10) |
where the more favorable constraint (7) has been used. A primordial field wound up by differential rotation ultimately decays: In a region with closed streamlines (a galaxy in this case) this effect is known as flux expulsion (Moffatt 1978).