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0 correspond to values of β≈0.9 which would be inconsistent with the results of other physical techniques, whereas the values of β≈0.6 we obtain for these ESR spectra with the dynamic cage model fits are consistent, as we have shown above.
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c is characteristic of the incipient smr, which is actually quite broad. A restricted distribution, covering the incipient smr to deep into the smr would still be a broad superposition and not have the distinctive two-component features seen experimentally, [cf. Fig. 1(b)].
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