Effects of very weak magnetic fields on radical pair reformation.
We can expect that biological responses to very weak ELF electromagnetic fields will be masked by thermal noise. However, the spin of electrons bound to biologically important molecules is not strongly coupled to the thermal bath, and the effects of the precession of those spins by external magnetic fields is not bounded by thermal noise. Hence, the known role of spin orientation in the recombination of radical pairs (RP) may constitute a mechanism for the biological effects of very weak fields. That recombination will generally take place only if the valence electrons in the two radicals are in a singlet state and the effect of the magnetic field is manifest through differential spin precessions that affect the occupation of that state. Because the spin relaxation times are of the order of microseconds, any effects must be largely independent of frequency up to values of a few megahertz. Using exact calculations on an appropriately general model system, we show that one can expect small, but significant, modifications of the recombination rate by a 50 microT field only under a narrow range of circumstances: the cage time during which the two elements are together must be exceptionally long--of the order of 50 ns or longer; the hyperfine field of either radical must not be so great as to generate a precession period greater than the cage containment time; and the characteristic recombination time of the radical pair in the singlet state must be about equal to the containment time. Thus, even under such singularly favorable conditions, fields as small as 5 microT (50 milligauss) cannot change the recombination rate by as much as 1%. Hence, we conclude that environmental magnetic fields much weaker than the earth's field cannot be expected to affect biology significantly by modifying radical pair recombination probabilities.
Adair
R K
RK
Department of Physics, Yale University, New Haven, Connecticut 06520-8121, USA.
D000465:Algorithms; D004574:Electromagnetic Fields; D004578:Electron Spin Resonance Spectroscopy; D004583:Electrons; D004735:Energy Transfer; D006358:Hot Temperature; D006801:Humans; D006859:Hydrogen / Q000528:radiation effects; D006860:Hydrogen Bonding / Q000528:radiation effects; D008280:Magnetics; D008956:Models, Chemical; D013997:Time Factors
D006859:Hydrogen