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Peak Position, cm * Intensity. Width, cm * Integral.

8929 03 9 3207 1330

11220 0.60 2673 1926

13378 0.41 2956 1281

15567 0.31 3517 1162

This would mean that the crystal field transitions would have very similar

energies. Given the widths o f the two bands, (3207cm*^ and 2672cm \ respectively),

it is likely that there are a number o f crystal field bands superimposed on one another,

arising fi-om the 'Tjg transition o f Fe^^ in all three o f the cation sites, and that

the curve fitting program cannot resolve the other peaks. This was found to be a

problem by Keppler et al. (1995) in their study o f (N%, Fe)Si03 perovskite.

An accurate energy level diagram for any o f the three cation sites would be

hard to work out because o f this superposition o f peaks, and, therefore no attenpt has

been made to derive one. However, some idea o f the crystal field parameters can be

obtained if two assumptions are made. The first assumption is that the two curves

fitted to the spectrum can be taken as averages o f the peaks due to the crystal field

transitions. From this, the position o f the baricentre o f the eg orbitals can be obtained.

For the single crystal o f wadsleyite at OGPa, the position o f the baricentre is 10075cm'

\ The second assumption concerns the sphtting o f the tzg orbitals. From Table 6.1, it can be seen that for a wadsleyite with 16% Fe, the quadratic elongation parameter

ranges fi*om 1.0053 to 1.0066. As a comparison, the quadratic elongation o f the cation

site in ringwoodite is 1.0005 (Bums, 1993). Bums and Sung (1978) suggested that the

best estimate for the lower level sphtting in ringwoodite is lOOOcm'^ and given the

similarity in the distortions o f the sites in the wadsleyite and ringwoodite structures,

this is proposed to be a reasonable value for the sphtting in wadsleyite.

From this, a value for \ can be obtained, and for wadsleyite at OGPa, the octahedral sphtting is equal to 9575cm'\ This value can then be used to obtain the

CFSE o f the phase, as:

CFSE=Q . A A ^ +o (6.1)

wiiere a is equal to half the splitting between the orbitals. For the wadsleyite at

OGPa, the CFSE equals 4330cm \ In comparison, the values o f and CFSE for

fayalite olivine are 8883cm'^ and 4230cm'^ respectively for the M l site, and 8553cm'^

and 4158cm^ respectively for the M2 site, yielding average values o f 8718cm ^ for \

and 4194cm ^ for the CFSE. Ringwoodite has values for the crystal field parameters

o f 10763cm'^ and 4972cm'^ for \ and the CFSE. The values for the crystal field parameters are therefore much closer to those o f the fayalite than the ringwoodite.

The two remaining bands in the spectrum, at 13378cm'^ and 15567cm \ are

attributed to Fe^^ -^Fe^^ charge transfer, in agreement with the presence o f Fe^^^ in

the Mossbauer data wiiich is indicative o f IVCT. The widths o f the bands are also

characteristic o f IVCT transitions (Mattson and Rossman, 1987) and the position o f

the bands are close to those for other Fe^^ Fe^^ transitions in minerals containing

edge sharing octahedra (Table 6.3 and Bums, 1993). With the low concentration o f

FeP^ in the sample, the IVCT is likely to be o f type llIA, according to the

classification o f Day ( 1976) with the nature o f the sites involved in the charge transfer

being almost identical, finite clusters o f octahedra. The fact that more than one band

is seen is due to the nature o f the structure o f wadsleyite, which consists o f network

o f edge - sharing octahedra (Fig 6.1). The chains link in three ways: there are chains

o f M l - M2 octahedra parallel to b, double chains o f M3 octahedra parallel to a, and zig - zag chains involving all three octahedra running parallel to b and c. It is the charge transfer that causes the blue - green colour o f wadsleyite.

Mineral. Metal - metal distance, pm IVCr energy, cm'^ wadsleyite* M l - NG = 287; M l - M3 = 290 13378 M2 - M3 = 305; M3 - M3 = 280; 285 15567 wadsleyite^ 13374 15921 vivianite 285 15870 babingtonite 337 14710 andalusite 265 8 10900 290.1 13400 yoderite 290 13800 oithopyroxene M l - Ml = 315 M l - M2 = 308; 327 14500 calculated 2917 10570 o

Table 6.3: Coinpaiison o f ->Fe^^ charge üansfer eneigies. * denotes this study, ^ the work o f Ross (1996). All other data horn Bums (1993).

Polarised spectra were also obtained from single crystal sanples o f wadsleyite.

Fig. 6.4 shows a spectrum polarised parallel to the a - axis. A minhnum o f four curves

were required to fit this spectrum, as shown in Fig. 6.4, and the parameters for these

curves are given in Table 6.4. Assignments for these curves follow the arguments

given for the unpolarised spectrum, with the peaks at 8282 and 10370cm*^ being due

to the crystal field transitions o f Fe^^ in the M l, M2 and M3 sites in the structure, and

the peaks at 13372 and 16137cm^ being attributed to IVCT. These IV C I bands are

due to the double chains o f M3 octahedra

A spectrum polarised parallel to the b - axis is shown in Fig. 6.5. Again, a

minimum o f four curves were required to fit this spectrum, Miich is different to that

shown in Fig. 6.4. The curve fitting parameters are given in Table 6.5. Again, the

bands assignments follow that o f the unpolarised spectrum, with the two bands below

12000cm^ being crystal field bands o f Fe^^ and the bands at 13291 and 15187cm^

being due to the charge transfer processes involving the M l - M2 octahedral chains

and the ’zig - zag' chains.

Finally, Fig. 6.6 shows a spectrum polarised parallel to c - axis. Again, four

curves were fitted to the spectrum, and the parameters are given in Table 6.6. Hie

spectrum itself is slightly broader than the other polarised spectra, and one o f the

charge transfer peaks, lying at 14113cm'^ is exceptionally weak in comparison to the

other charge transfer peaks recorded above. This is due to there being only one form

o f charge transfer along the c - axis, involving the 'zig - zag' chains as described

above.

What is noticeable from all the polarised spectra is that there is charge transfer

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Wavenumber cm*