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Management of Commercially Generated Radioactive Waste - U.S. ...

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P. 10<br />

appropriate host phases. The main criteria are similarity <strong>of</strong> chemical parameters, particu-<br />

larly the ionic radius and the charge. Other parameters such as polarizability and<br />

d-orbital interactions will have a lesser effect in determining the amount <strong>of</strong> substitution.<br />

Thus one can use a table <strong>of</strong> ionic radii to predict possible substitutions, remembering that<br />

charge balance must be maintained by a coupled substitution <strong>of</strong> another element whenever<br />

necessary.<br />

P.1.3.2 Ionic Radii<br />

Table P.1.6 lists the ionic radii <strong>of</strong> the important nuclear waste elements and <strong>of</strong> the<br />

elements present in minerals which are most likely to be substituted. Usually, complete<br />

substitution may occur if the ionic radii differ by no more than 15%. Limited substitution<br />

may occur if the radii difference is larger, or a new compound may be induced to form. This<br />

compound may be isostructural with the host phase or may have a distinctly different struc-<br />

ture. If the phase is isostructural, then stability properties <strong>of</strong> the new phase may be<br />

similar to that <strong>of</strong> the host, or certainly be close enough to warrant further investigation.<br />

TABLE P.1.6 Selected Ionic Radii(a)<br />

Ion CN(b) Ionic Radius (A) Ion CN Ionic Radius (A)<br />

Cs +<br />

Sr 2+<br />

1 +<br />

X 1.81 Na<br />

VI 1.02<br />

VIII 1.25 IX 1.32<br />

11- VI 2.20 K 1 + VI 1.38<br />

15+ VI 0.95 IX 1.55<br />

Tc 4+<br />

Tc 7+<br />

VI 0.65 Ca 2 + VI 1.00<br />

VI 0.56 VIII 1.12<br />

La 3+ VIII 1.16 Ba 2 + VI 1.36<br />

VIII 1.42<br />

3 +<br />

Dy<br />

4 +<br />

Ce<br />

4 +<br />

U<br />

6 +<br />

U<br />

4 +<br />

Np<br />

Pu3 +<br />

4 +<br />

Pu<br />

3 +<br />

Am<br />

Am 4<br />

3 +<br />

Cm<br />

VIII 1.03 C1 1 - VI 1.81<br />

VIII 0.97 Br 1 - VI 1.96<br />

VIII 1.00 Y3+ VIII 1.02<br />

II 0.45 Zr 4 _ VIII 0.84<br />

VIII 0.98 Ti 4+ VI 0.61<br />

VI 1.00 Th 4 VIII 1.04<br />

VIII 0.96 Mn3+(HS)(c) VI 0.65<br />

VI 1.00 Fe3+(HS) VI 0.65<br />

VIII 0.95 Cr 3<br />

VI 0.62<br />

VI 0.98 Ce 3 + VIII 1.11<br />

(a) After Shannon and Prewitt (1969).<br />

(b) CN = coordination number.<br />

(c) HS = high spin.

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