Neutrinos with a magnetic moment mu change their helicity when interac
ting with an electromagnetic field. Various aspects of this effect hav
e been described as spin precession, spin-flip scattering, and magneti
c Cherenkov radiation, These perspectives are unified in an expression
for the nu(L)-->nu(R) transition rate which involves the correlators
of the electromagnetic field distribution, Our general formula correct
s a previous result and generalizes it to the case where the fields ca
nnot be viewed as classical and where the momentum transfers need not
be small, We evaluate our result explicitly for a relativistic QED pla
sma and determine the depolarization rate to leading order in the fine
structure constant, Assuming that big-bang nucleosynthesis constraint
s do not allow a right-handed neutrino in equilibrium we derive the li
mit mu < 6.2 x 10(-11) mu(B) on the neutrino magnetic moment. Bounds o
n mu from a possible large scale magnetic fields are found to be more
stringent even for very weak fields. (C) 1997 Elsevier Science B.V. PA
CS: 98.80; 13.15.