ISSN 0036-0236, Russian Journal of Inorganic Chemistry, 2009, Vol. 54, No. 2, pp. 294–298. © Pleiades Publishing, Ltd., 2009.
Original Russian Text © I.Ya. Zaitseva, I.S. Kovaleva, V.A. Fedorov, 2009, published in Zhurnal Neorganicheskoi Khimii, 2009, Vol. 54, No. 2, pp. 338–343.
PHYSICOCHEMICAL ANALYSIS
OF INORGANIC SYSTEMS
Glass Formation in the HgBr2–PbBr2–CsBr Ternary
I. Ya. Zaitseva, I. S. Kovaleva, and V. A. Fedorov
Kurnakov Institute of General and Inorganic Chemistry, Russian Academy of Sciences,
Leninskii pr. 31, Moscow, 119991 Russia
Received February 14, 2008
Abstract—Results of investigation of glass formation in the HgBr2–PbBr2–CsBr system are presented. The
glass formation region has been outlined. Characteristic temperatures have been determined by differential ther-
mal analysis, and the ratio Tg/Tm and factor HR have been calculated for vitreous samples of the HgBr2–PbBr2–
CsBr ternary.
DOI: 10.1134/S0036023609020223
Increased interest observed currently to bromide investigated three samples with compositions close to
ternary eutectics Ö2, Ö3, and Ö4 (Fig. 1). Quenching of
these samples showed that they are vitreous [3]. In [4],
we presented the results of the investigation of glass
formation along three joins: of the HgBr2–PbBr2–CsBr
ternary system CsHgBr3–CsPbBr3 (1), Cs2HgBr4–
CsPbBr3 (2), and CsHg2Br5– CsPbBr3 (3). Quenching
gave glassy samples in the following ranges: along
join 1, over the whole concentration range; along
join 2, within 8.7–100 mol % CsPbBr3; and along
join 3, within 0–40 and 70–100 mol % CsPbBr3. The
compositions of the most stable glasses along joins 1–3
were near the eutectic compositions, which confirmed
the relation of the liquidus temperature with the glass-
forming tendency in systems.
compounds in both crystalline and vitreous states is due
to the possibility of their use in IR optics because of
their transparency in the far-IR spectral region (above
20 µm) [1]. We choose to study the ternary system con-
sisting of mercury, lead, and cesium bromides because
cations of heavy metals shift the absorption band edge
to a long-wavelength region, which is important to the
use of such materials in IR engineering.
The purpose of this work was to investigate glass
formation in the HgBr2–PbBr2–CsBr ternary system.
We previously investigated interactions in binary sys-
tems bordering the HgBr2–PbBr2–CsBr system. In the
HgBr2–CsBr and PbBr2–CsBr systems, compounds
CsHg2Br5, CsHgBr3, Cs2HgBr4, CsPb2Br5, CsPbBr3, and
Cs4PbBr6 are formed; two of them (CsPb2Br5 and
Cs4PbBr6) melt incongruently. As a result of the investi-
gation of interactions in the mentioned ternary system,
we outlined the fields of primary crystallization of
phases, determined the coordinates of ternary invariant
points, and lined isotherms [2]. These data were used in
the investigation of glass formation in the ternary sys-
tem since it is known that samples with the composi-
tions close to eutectic ones have a larger ability to glass
formation. First, we investigated glass formation in
binary systems bordering the HgBr2–PbBr2–CsBr ter-
nary system. Upon quenching samples to an ice–water
mixture at ~100–150 K/s in the CsBr–HgBr2 system,
we obtained glasses in the concentration range of 46–
76 mol % HgBr2; in the CsBr–PbBr2 system, in the
concentration range of 50–95 mol % PbBr2; and in the
HgBr2–PbBr2 system, no glasses were obtained. Of the
six ternary compounds of the HgBr2–PbBr2–CsBr sys-
tem, only two, namely, Cs2HgBr4 and Cs4PbBr6, were
not obtained in a vitreous state. To determine glass for-
mation in the HgBr2–PbBr2–CsBr ternary system, we
To restrict the glass formation region in the HgBr2–
PbBr2–CsBr ternary system, in this work, we addition-
ally studied three joins, namely, the polythermal iso-
concentration join with 40 mol % HgBr2 (4), HgBr2–
CsPbBr3 (5), and CsHgBr3–PbBr2 (6), as well as
some samples of the ternary system.
EXPERIMENTAL
To investigate glass formation in the HgBr2–PbBr2–
CsBr system, as starting substances, we used HgBr2
synthesized as in [5], high-purity grade PbBr2, and
chemically pure grade CsBr dried at 100°ë to remove
trace water. The melting points of HgBr2, PbBr2, and
CsBr determined by DTA were 245, 360, and 640°ë,
respectively. The CsPbBr3 and CsHgBr3 compounds
necessary for the investigation of glass formation along
joins 5 and 6 were prepared from dried mercury, lead,
and cesium bromides in silica cells evacuated to a resid-
ual pressure of 10–3 Pa at 640°ë for 1 day under stirring,
annealed for 3 days at 200°ë, and then cooled in the
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