2009
DOI: 10.1039/b907915g
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Radiofrequency polarization effects in low-field electron paramagnetic resonance

Abstract: Low-field optically detected EPR spectra of photochemically formed transient radical ion pairs are reported for weak circularly and linearly polarized radiofrequency (RF) fields. The spectra are found to be strongly dependent on the polarization and frequency of the RF field and on the angle between the static magnetic field and the plane containing the RF field. The spectra are discussed in terms of resonances arising from Zeeman and hyperfine interactions; the conditions for validity of the rotating frame ap… Show more

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Cited by 10 publications
(25 citation statements)
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“…5 In the high-field limit it is convenient to make the rotating frame approximation in order to remove the time-dependence of the problem. Such an approximation cannot be used in the low-field limit 6 or when the static and oscillating fields are not orthogonal. A modified form of the γ-COMPUTE algorithm [11][12][13] is used which exploits the periodicity of the problem and efficiently averages over the initial phase of the RF field.…”
Section: Simulation Methodsmentioning
confidence: 99%
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“…5 In the high-field limit it is convenient to make the rotating frame approximation in order to remove the time-dependence of the problem. Such an approximation cannot be used in the low-field limit 6 or when the static and oscillating fields are not orthogonal. A modified form of the γ-COMPUTE algorithm [11][12][13] is used which exploits the periodicity of the problem and efficiently averages over the initial phase of the RF field.…”
Section: Simulation Methodsmentioning
confidence: 99%
“…[4][5][6] The breakdown of high-field models is gradual, parallel transitions becoming significant at higher frequencies than those at which the rotating frame approximation breaks down. 6 Extending previous studies, orientation effects are now investigated in the case of strong B 1 fields.…”
Section: Orientation-dependent Effectsmentioning
confidence: 99%
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