12.01.2013 Views

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

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

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

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Qv ==<br />

,<br />

2<br />

28 kHz<br />

-111-<br />

which is slightly larger than the width of the vanadium resonance<br />

line. That the origin of this large linewidth was mainly quadrup-<br />

olar in origin was made evident by the large quadrupolar echoes<br />

observed following for example a 90-T-35 pulse sequence<br />

(118,119)ý<br />

As expected, rapid sample rotation about the magic angle at speeds<br />

of around 5 kHz failed to have any effect upon the nuclear lineshape.<br />

There are very few compounds of niobium which can be observed<br />

by NMR. The niobium Knight shift has been measured previously<br />

with respect to Nb205 dissolved in hydrofluoric acid. However in<br />

our work the Knight shift was determined against a solution of<br />

NbC15 in pure acetone. The solution is light yellow upon the<br />

NbC15 first being introduced, but later turns brown and produces<br />

a brown precipitate. Although the 93Nb resonance observed during<br />

this time varies considerably both in frequency and in T2, after<br />

several hours it becomes constant. The Knight shift value obtained<br />

by direct substitution of the reference and metal samples into<br />

the Bruker coil was 0.768 ± 0.0087. Values quoted in the literat-<br />

ure with respect to Nb205 in HF are 0.85(120) and 0.875%(127)<br />

view of the unknown nature of the reference compounds, the discrep-<br />

ancy is not meaningful.<br />

The large experimental Knight shifts measured for both vanadium<br />

and niobium have been explained'in terms of a large orbital contrib-<br />

ution to the hyperfine coupling in these two metals(123).<br />

.<br />

In

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!