Journal of Alloys and Compounds 471 (2009) 60–63
Journal of Alloys and Compounds
journal homepage: www.elsevier.com/locate/jallcom
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The isothermal section of the Ce–Co–Sb ternary system at 400 C
∗
R.M. Luo, F.S. Liu, J.Q. Li , X.W. Feng
College of Materials Science and Engineering, Shenzhen University and Shenzhen Key Laboratory of Special Functional Materials,
Shenzhen 518060, PR China
a r t i c l e i n f o
a b s t r a c t
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Article history:
Phase equilibria were established in the Ce–Co–Sb ternary system at 400 C based on X-ray powder
diffraction (XRD), scanning electron microscopy (SEM) and energy dispersion spectroscopy (EDS) tech-
niques. Fourteen binary compounds Ce24Co11 , CeCo2, CeCo3, Ce2Co7, Ce5Co19 , Ce2Co17 , CoSb, CoSb2, CoSb3,
Ce2Sb, Ce5Sb3, Ce4Sb3, CeSb and CeSb2 have been confirmed, and three ternary compounds CeCoSb3,
Received 7 December 2007
Received in revised form 12 March 2008
Accepted 12 March 2008
Available online 9 May 2008
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CeCo1−xSb2 and CeCo1.33 Sb2 are found in this system at 400 C. The isothermal section of this sys-
tem at 400 C consists of 20 single-phase regions, 40 two-phase regions and 21 three-phase regions.
The compound CeCo1−xSb2 has ZrCuSi2-type structure with space group P4/nmm, a = 0.3878 nm and
c = 0.9849 nm. The crystal structure for the compound CeCoSb3 is determined to be CeNiSb3-type (Pbcm)
with a = 1.27697 nm, b = 0.60601 nm and c = 1.8435 nm. The compound CeCo1.33 Sb2 is of orthorhombic sys-
tem with a = 0.6083 nm, b = 0.60118 nm and c = 1.04596 nm. The homogeneity range of CoSb phase is about
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Keywords:
Rare earth alloys and compounds
Phase diagram
X-ray powder diffraction
2
at.%. The solubilities for the other single-phase regions were not observed.
©
2008 Elsevier B.V. All rights reserved.
1
. Introduction
alloys were re-melted two or three times in order to achieve complete fusion and
homogeneous composition. All samples were subjected to annealing for homoge-
nization in evacuated quartz ampoules in a resistance furnace. The homogenization
temperatures of the alloys were chosen on the basis of the binary phase diagrams of
The Co–Sb system is drawing more and more attention due to
its special feature found in recent years. The compound CoSb3 in
this system has the typical skutterudite structure exhibiting excel-
lent transport properties, such as extremely high carrier mobility,
that are desirable for good thermoelectric performance [1,2]. Rare
earth-filled skutterudites have been identified as potential thermo-
electric materials due to their reduced thermal conductivity [3,4].
Understanding the phase relationships of Re–Co–Sb system is help-
ful for the development of relative materials. The investigations of
phase diagrams of the Eu–Co–Sb [5], Gd–Co–Sb [6], Nd–Co–Sb [7]
and Pr–Co–Sb [8] have been reported, while no reports have been
found on the interaction in the Ce–Co–Sb ternary systems. In this
work, we investigated the phase equilibria in the Ce–Co–Sb ternary
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the Ce–Sb, Ce–Co and Sb–Co systems. The homogenization was performed at 600 C
for 20 days for the samples containing equal to or more than 40 at.% Sb, while at
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900 C for 15 days for the samples containing less than 40 at.% Sb. They are all then
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cooled to 400 C at the rate of 10 C/min, kept at 400 C for 3 days and subsequently
quenched into liquid nitrogen. 118 alloy samples in total were prepared for this
investigation.
The treated alloys were powdered for X-ray powder diffraction (XRD) analy-
sis. The phases in each alloy were identified by XRD with Cu K␣ radiation (Bruker,
D8 Advance SS 18 kW) and JADE 5.0 software. The software Topas 3.0 was used for
Rietveld refinement [9]. The morphology and composition of the phase were inves-
tigated using a cold field emission scanning electron microscope (SEM) with energy
dispersive analysis (EDS) (HITACHI S-4700).
3. Results and discussion
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system at 400 C.
3.1. Phase analysis
2.
Experimental detail
Cerium (purity of 99.99%), antimony (purity of 99.95%) and cobalt (purity of
9.99%) were used as raw materials. The alloys with 40 at.% Sb or more were pre-
We have studied the binary systems Co–Sb, Ce–Co and Ce–Sb
at 400 C to identify the binary compounds. The X-ray diffraction
9
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pared by high frequency melting under a high purity argon in quartz tube which
was first evacuated to high vacuum to avoid the weight lost of the samples owing to
the high volatility of antimony. The alloys with the Sb content less than 40 at.% were
a water-cooled copper tray under the protection of a pure argon atmosphere. The
analysis confirmed the existence of the 14 binary compounds in
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the Ce–Co–Sb ternary system at 400 C: Ce24Co , CeCo , CeCo ,
11
2
3
Ce2Co7, Ce5Co19 and Ce2Co17 in the Ce–Co system; CoSb, CoSb2
and CoSb3 in the Co–Sb system; Ce Sb, Ce Sb , Ce Sb , CeSb and
2
5
3
4
3
CeSb2 in the Ce–Sb system. The binary compounds found in this
work are in well agreement with those compounds reported in
the literatures for Ce–Co [10], Co–Sb [11] and Ce–Sb [12] binary
systems. The structure types and lattice parameters of these com-
∗ Corresponding author. Tel.: +86 755 26538528; fax: +86 755 26536239.
0925-8388/$ – see front matter © 2008 Elsevier B.V. All rights reserved.
doi:10.1016/j.jallcom.2008.03.061