Chemistry Reference
In-Depth Information
This interpretation could justify why some of the compounds listed in Table
5
produce ilmenites and rutiles as sub-products of decomposition. We will see later
that the appearance of perovskites can also be explained.
8.2 Extension to Mn
2
GeO
4
: The Olivine-,
Spinel- and Sr
2
PbO
4
-Type Structures
Mn
2
GeO
4
crystallizes in three polymorphs. At ambient conditions it is olivine-like
(
first one is a tetragonal spinelloid
P
b
-phase (
I
mma), transforming at higher pressures
into the Sr
2
PbO
4
-type structure (
bam).
Although Mn
2
GeO
4
is isostructural with Ca
2
SnO
4
, a detailed discussion of its
structure will doubtless clarify many of the peculiarities discussed about Ca
2
SnO
4
.
The relationships that can be established between the cation subarray of Ca
2
SnO
4
and the corresponding Ca:Sn alloys will be of special importance.
In the Ca-Sn system, two phases have been reported. The first one is Ca
2
Sn
P
(
pressure-induced CrB
P
formulate the compound as (CaO)
2
SnO
2
.
We have seen that the existence of blocks of a bixbyite-type structure was
interpreted as if a II-IV compound (CaSn) was chemically equivalent to a III-III
subarray, such as elemental indium. Thus, (CaO)CaSnO
3
should be equivalent to
CaO(
!
-In
2
O
3
are fragments of real
C
-In
2
O
3
(also
C
-Sc
2
O
3
).
Thus, the equivalence between the CaSn subarray and the In structure is evident.
Ca
2
SnO
4
can also be compared with the Ca
2
Sn alloy. The latter is anti-PbCl
2
,
whereas the oxide stabilizes a Ca
2
Sn subarray which could not be related to any
known alloy. This was the reason why, in the above section, the Ca
2
Sn substructure
was fragmented to find relationships with other structures.
This feature contrasts with that shown by the related compounds Ca
2
Ge and
Ca
2
SnO
4
(Sr
2
PbO
4
type) in terms of the
equivalence oxidation-pressure
. Because
the Ca
2
Sn subarray is anti-PbCl
2
type, it should be expected that, when oxidized,
the Ca
2
Sn subarray should necessarily undergo the complete transition series Ni
2
Si
!
C
-In
2
O
3
), in which
C
Ca
2
Sn
. Of these, only the initial and the final states
have been identified, the former for Ca
2
Sn and the latter in Ca
2
SnO
4
. This implies
that Ca
2
Sn is forced to undergo the direct transition Ni
2
Si to Ca
2
Sn[O
4
].
ture, it transforms into a Ca-stuffed wurtzite-like network of composition CaGeO
4
,
able as Ca
2+
[
Ni
2
In
!
TiSi
2
!
MgCu
2
!
-Ge
2
O
4
], as Ni
2
In type and finally as Mo
2
Si type, which is the
structure type of the Ba
2
Sn subarray in Ba
2
SnO
4
.
C