Exact analytical expressions for the evolution of a non-diffusing spin
-correlated radical pair in a strong magnetic held are presented. The
recombination of singlet and triplet pairs at different rates, and the
coherent evolution caused by magnetic interactions, lead to radical p
air concentrations which are the sum of four time-dependent terms: two
decaying exponentials and two exponentially damped oscillations. The
predicted time dependence is used to illuminate the recombination dyna
mics of the primary radical pair in photosynthetic bacterial reaction
centres. Although mono-exponential decay is expected similar to 20 ns
after the formation of each individual radical pair, the inhomogeneous
distribution of Larmor frequencies of the two electron spins leads to
non-exponential kinetics and different time constants for the disappe
arance of singlet and triplet pairs, and the formation of singlet and
triplet recombination products.