An improved semiclassical theory of radical pair recombination reactions
David E. Manolopoulos, P. J. Hore

TL;DR
This paper introduces a practical semiclassical method for simulating electron spin dynamics in radicals with many nuclear spins, improving accuracy over previous models and enabling analysis of large, complex systems.
Contribution
The new method allows individual nuclear spins to precess around the electron spin, providing more accurate long-time behavior predictions and applicability to larger radicals.
Findings
Method scales linearly with nuclear spins
Achieves quantitative agreement with quantum mechanics as system complexity increases
Correctly predicts low magnetic field effects in radical recombination
Abstract
We present a practical semiclassical method for computing the electron spin dynamics of a radical in which the electron spin is hyperfine coupled to a large number of nuclear spins. This can be used to calculate the singlet and triplet survival probabilities and quantum yields of radical recombination reactions in the presence of magnetic fields. Our method differs from the early semiclassical theory of Schulten and Wolynes [J. Chem. Phys. 68, 3292 (1978)] in allowing each individual nuclear spin to precess around the electron spin, rather than assuming that the hyperfine coupling-weighted sum of nuclear spin vectors is fixed in space. The downside of removing this assumption is that one can no longer obtain a simple closed-form expression for the electron spin correlation tensor: our method requires a numerical calculation. However, the computational effort increases only linearly with…
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