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NNR IN RAPIDLY ROTATED METALS By - Nottingham eTheses ...

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- 118 -<br />

Lifetime broadening alone gives rise to a Lorentzian line-<br />

shape in the frequency domain with a width at half-height of 1/'nT1.<br />

Assuming that the lifetime contribution to the total width of the<br />

residual spectrum can be separated by a simple subtraction, then<br />

upon substituting the values for T1 recorded previously the secular<br />

broadening of the central line becomes about 560 Hz for both iso-<br />

topes. The above value includes a contribution from the inhomo-<br />

geneity of the magnetic field but this was estimated to be negigible<br />

(< 20 Hz) in comparison. Consequently the figure quoted represents<br />

a measure of the electron coupled scalar interaction between the<br />

cadmium nuclei. The equivalence of the linewidth for the two iso-<br />

topes simply reflects their almost equal natural abundancies.<br />

At room temperature the relaxation times of both isotopes are of<br />

approximately the same magnitude as the inverse of the first and<br />

second nearest neighbour exchange coupled constants as determined<br />

(139)<br />

by Alloul and Deltour. This leads to the possibility that<br />

the isotropic magnetic exchange interaction may be time averaged by<br />

lifetime fluctuations in the nuclear spin states. Any detailed<br />

calculation of the Rudermann-Kittel(14) indirect exchange interact-<br />

ion is precluded by an incomplete knowledge of the effect of these<br />

fluctuations as well as by the preliminary nature of the results.<br />

Consequently we content ourselves with making a simple comparison<br />

of our results to those obtained by Alloul and Deltour from observat-<br />

ion of the modulated structure of the spin echoes of the 113Cd reson-<br />

ance in cadmium based alloys. Their experiment was undertaken at<br />

liquid helium temperatures, in which region T1 contributions to the<br />

lineshapes are negligible. The exchange coupling constants, J1<br />

and J2, between the first and second nearest neighbours in the hexagonal

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