NEUTRINO MASS AND THE ORIGIN OF GALACTIC MAGNETIC-FIELDS

We compare two constraints on the strength of the cosmological primord ial magnetic field: the one following from the restrictions on the Dir ac neutrino spin flip in the early Universe, and another one based on the galactic dynamo theory for the Milky Way (presuming that the seed magnetic field has a relic origin). Since the magnetic field facilitat es transitions between left- and right-handed neutrino states, thereby affecting He-4 production at primordial nucleosynthesis, we can obtai n a guaranteed upper limit on the strength of the relic magnetic field in the protogalaxy, B(c) less than or similar to 4 X 10(-9)-3 X 10(13 ) G, depending on the neutrino magnetic moment, if we adopt the MSW ex planation of the GALLEX results. On the other hand, models of the dyna mo in the Milky Way indicate that the seed magnetic field should be at least 10(-11)-10(-13) G at the protogalaxy scale L = 100 kpc. These u pper and lower limiting ranges are marginally consistent provided the electron neutrino mass is below 0.3 eV. The results apply to a relic m agnetic field produced in the early Universe by any causal mechanism b efore the nucleosynthesis.